The galaxy appears to be an elliptical galaxy. It exhibits a smooth, centrally concentrated luminosity profile, with a lack of defined spiral arms or prominent dust lanes. The central region displays a bright yellowish hue, potentially indicating an older stellar population. Moving outward, the color transitions to a slightly bluer tint. The galaxy's overall shape is elongated with moderate ellipticity. There is no obvious indication of tidal disturbances or ongoing major mergers. There is a hint of minor asymmetry in the outer regions which could be indicative of a potential minor merger.