This galaxy exhibits a disturbed morphology, possibly indicative of an ongoing or recent interaction. There appears to be a central bulge of concentrated luminosity, yellowish in color, which may suggest an older stellar population. Extending away from the central bulge are fainter, bluish features, hinting at younger stars or areas of active star formation. The overall shape is irregular and elongated, which is not consistent with a classical spiral or elliptical morphology, supporting the hypothesis of a merger or tidal disruption. The galaxy shows moderate luminosity and redshift, suggesting that it is a relatively small galaxy at a moderate distance.
