This galaxy appears to be a late-stage merging system or interacting system. It presents a generally elliptical or lenticular morphology. The central bulge appears bright and somewhat spheroidal. The galaxy exhibits features indicative of tidal disruption or interaction, manifesting as faint plumes or extensions of stellar material extending outwards from the main body, which could have come about due to an ancient minor merger. The galaxy exhibits a blue hue in the outer regions with an orange or yellow color in its center, which is suggestive of recent or ongoing star formation in the disc and an older stellar population concentrated in the center of the galaxy. There is some evidence of distortion in the shape of the galaxy, likely resulting from gravitational interactions with a past or present companion. Overall, it appears as a system in a state of transformation or merging, with ongoing star formation in some regions and older stellar populations in others.
