The galaxy presents a largely smooth morphology, suggesting a likely classification as an elliptical or lenticular galaxy. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards the outer regions. The shape appears to be generally rounded. There is faint bluer emission extending away from the center, indicating a low level of on-going star formation. There is no distinct, strong tidal feature indicative of an ongoing major merger, although some slight asymmetries are present, possibly pointing towards a minor interaction or internal disturbance. Overall, the galaxy presents a relatively quiescent, evolved appearance.
