The galaxy appears as a relatively smooth, elliptical object. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color distribution suggests a dominant older stellar population, with reddish hues more prominent in the core and a slight shift towards bluer tones in the surrounding halo. There is no apparent disk or spiral arm structure. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, it looks like it is in a relatively relaxed state.
