The galaxy appears to be a relatively small, elliptical galaxy. It exhibits a smooth, concentrated light profile, with the majority of its light concentrated in the central region. There is no obvious spiral structure or disk component visible in this image, with no apparent features or irregularities, such as tidal tails or strong dust lanes, suggesting it has not undergone a major merger recently. The core is somewhat spherical. The color index suggests a population of older stars. This is consistent with a low star formation rate for this galaxy. 