Fig. 1
2.′2 × 1.′8 V-band image of FM 287-14. Top: the huge visible halo. shells and a tidal filament, enhanced by a 500-pixel2 median kernel filtering of the original image. Bottom: the same image in a different contrast: (1) the bulge and the central region; (2) a ring-like structure surrounding the bulge; and (3) a partial outer ring spreading to the N direction, which may be the locus of intense star formation within an underlying gaseous disk. See Table 5 for photometric measurements of the numbered regions.
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