The galaxy presents as a slightly inclined spiral, exhibiting a moderately smooth overall structure. There is a distinct but not particularly well-defined central bulge, gradually fading into a disk component that lacks tightly wound or prominent spiral arms. The disk appears somewhat flocculent, indicating a degree of ongoing star formation, and a slightly disturbed appearance, hinting at potential past or ongoing interactions or internal dynamics. It exhibits a moderate color index, trending towards a slightly redder hue. The apparent size is relatively small, suggesting it is a dwarf galaxy. There is evidence of some tidal features. Based on these observations, there appears to be a merger occurring.
