The galaxy presents a somewhat disturbed morphology, appearing elongated with a bright central region and a fainter, extended component suggestive of a tidal tail or debris field. The object's shape is far from circular; it is a flattened, elliptical form. The color distribution indicates variations in stellar populations across the galaxy; a redder hue appears to dominate the central bulge region, potentially indicating older stars, while bluer hues can be seen throughout the central disk. The galaxy is relatively small. The galaxy is at redshift z=0.107007, suggesting it is at a significant cosmological distance from our own. The galaxy appears to be undergoing some type of interaction, either a minor merger or some type of tidal disruption.
