The galaxy appears to be a relatively compact, elliptical galaxy, exhibiting a smooth, spheroidal morphology. The light is concentrated towards the center, which is bright and yellowish, suggesting an older stellar population is present. The outer regions gradually fade in intensity, with a subtle bluish tint in the surrounding halo. No prominent spiral arms or dust lanes are visible. There is no indication of any major ongoing merging events, although there is a minor disturbance that could be ongoing. Based on the color and lack of distinct features, star formation is likely occurring at a relatively low rate. The general appearance indicates a relatively old and quiescent system. The estimated size is roughly 4.4 kpc.