The galaxy presents as a centrally concentrated object with a noticeable bulge. The overall color appears somewhat redder in the central region, suggesting an older stellar population. The outer regions exhibit a bluer hue, which might indicate ongoing star formation. The morphology seems primarily smooth, although there are hints of a very faint, diffuse disk-like structure extending from the central bulge. The galaxy appears relatively isolated, showing no clear signs of any ongoing major mergers or significant tidal disturbances in this image. Overall, the galaxy seems to be a relatively evolved system with some residual star formation activity.
