The galaxy presents as a relatively smooth, elliptical-like morphology. It exhibits a centrally concentrated luminosity profile, with the light appearing most intense towards the core. The galaxy appears generally round in shape. There is some evidence of minor disturbance or perhaps tidal features suggesting a possible interaction or merger history, though the primary structure seems largely relaxed. There are no clearly defined spiral arms or a prominent disk component visible in the image. The overall color suggests an older stellar population and relatively low current star formation activity. The galaxy appears moderately luminous, indicating it is a reasonably massive system. There may be some dust lanes or patchy absorption features, but they are not particularly pronounced.
