The galaxy presents as an elliptical-like morphology, with a prominent central bulge exhibiting a yellowish hue. The color suggests a population of older, cooler stars dominating this region. Extending from this central region is a fainter, more diffuse component that shows a bluer color shift in the extended region. This suggests the presence of more active star formation within this region. There is some disruption in the disk, likely to be the result of an ongoing or recent merger. This galaxy exhibits signs of past merger activity, with some indications of tidal features. The galaxy has a moderate size in the observed field.
