The galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. The primary body appears to be a relatively smooth spheroid, potentially an elliptical galaxy or the bulge component of a spiral. It exhibits a yellowish-red hue, indicating an older stellar population, with minimal ongoing star formation. A distinct tidal feature extends from the main body, appearing as a bluish elongated structure. This suggests a significant tidal interaction, possibly with another galaxy or a smaller dwarf galaxy that has since been disrupted. The blue color of this structure is indicative of recent star formation activity, likely triggered by the gravitational interaction. A smaller, yellowish structure is also connected to the other side of the spheroid. There is a faint arc on the bottom of the galaxy, also possibly indicative of tidal forces from a merger. The galaxy is neither strongly disturbed nor completely relaxed, indicating that the system is likely in a state of transition following a merging event.
