The galaxy presents a generally smooth morphology, with a predominantly elliptical shape. The light distribution is centrally concentrated, displaying a gradual decrease in intensity from the core outwards. There is a lack of discernible spiral arm structures or prominent dust lanes, suggesting a classification towards early-type galaxies, possibly an elliptical or lenticular galaxy.

Color gradients indicate a bluer outer halo and a redder center. This color variation potentially corresponds to variations in stellar population, with the core being dominated by older, redder stars. The slight color differences may also be from mild ongoing star formation in the outer edges or halo, but this is difficult to conclude due to lack of resolved detail. There is no indication of any merging activity or tidal disturbances present in the image. The galaxy appears to be relatively isolated and undisturbed.
