The galaxy appears to be an elliptical type, characterized by a largely featureless, smooth profile. The light distribution suggests a high degree of central concentration, with intensity decreasing steadily outwards from the core. The galaxy appears circular in projection. There is a slight color gradient, with the central region appearing yellower than the outer regions, which may indicate an older stellar population in the core. No distinct spiral arms, bars, or dust lanes are discernible. There is no indication of any tidal features or ongoing merger activity.
