The galaxy presents as a relatively smooth, elliptical or lenticular structure with a concentrated central bulge. There is a subtle color gradient visible, with the central region appearing slightly more yellow-red compared to the outer regions, which exhibit a bluer hue. This suggests a population of older stars concentrated in the core, with the presence of younger, bluer stars in the disk or outer regions. The galaxy shows no obvious signs of ongoing major mergers or strong tidal disturbances, however there is a very slight asymmetry that could indicate a possible minor disturbance. The shape is mostly in between rounded and elongated. The galaxy is estimated to have a moderate star formation rate. The estimated size is roughly 8 kpc in radius.