The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, indicative of a substantial stellar population. The light appears to fade gradually outwards with the distribution of stars being fairly uniform. There is no apparent spiral arm structure or significant dust lane obscuration. The galaxy's shape appears generally round, with only a slight deviation towards an elongated form. There is no obvious evidence of tidal tails, bridges, or other major disturbances suggesting recent or ongoing major merger activity. There appears to be some subtle asymmetry in the outer isophotes, potentially hinting at minor gravitational interactions or past merger events. Colors appear to be in the yellowish range.
