The galaxy appears to be a relatively smooth, concentrated object, likely an elliptical or lenticular galaxy, viewed at a distance where finer details are not readily discernible. It presents a centrally condensed light profile, with a gradual decrease in luminosity towards its outer edges. The overall color of the galaxy is slightly redder, suggesting a population of older stars and a relatively low rate of star formation. There might be a subtle hint of some minor structural disturbance or interaction with other nearby galaxies based on a slight asymmetry in its shape, though this could also be image noise or artifacts.
