The galaxy presents a relatively smooth, elliptical morphology with a slightly oblate spheroid shape. The core region exhibits a diffuse, concentrated luminosity. Moving outward, the light gradually diminishes without any sharply defined edges, implying a gradual decrease in stellar density. Evidence suggests ongoing or recent interaction with a smaller galaxy. A small feature extends from the main galactic body that suggests either tidal disruption or potentially a very small merging partner galaxy. The color distribution appears primarily yellow-orange, indicative of an older stellar population, but also some regions of blue, indicating more recent star formation, potentially spurred by the interaction with the smaller galaxy.
