The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated light profile, with the intensity peaking towards the center and gradually decreasing outwards. The color index indicates a population of older stars dominating the stellar content. There is little evidence of spiral arms or significant dust lanes. Its shape is consistent with a spheroidal system, approximately round in appearance. Faint tidal features may be present, suggesting past or ongoing interaction with another galaxy, although the possibility of these being artifacts cannot be discounted. The galaxy is not currently undergoing significant star formation, appearing quiescent in nature. No prominent central active galactic nucleus is discernible from the data.