The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated light profile, with a gradual decrease in luminosity moving outwards from the core. The color index suggests a redder population of stars, implying an older stellar population. There is little to no evidence of spiral arms or significant dust lanes. The shape appears generally round. There is no indication of tidal tails or other major disturbances indicative of an ongoing or recent merger event. The overall appearance suggests a quiescent galaxy with a relatively low star formation rate.
