The galaxy presents as a relatively smooth, centralized object with a slight but noticeable disk-like structure. There is a pronounced central bulge that dominates the galaxy's overall luminosity. Color gradients suggest the presence of an older stellar population dominating the bulge. The disk, though subtle, shows a bluer coloration, which would indicate ongoing star formation compared to the redder bulge region. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances. There might be a slight asymmetry in the outer regions of the disk, possibly suggesting minor interactions or disturbances. The light is moderately concentrated, implying an intermediate stage in its evolutionary path. There is only a small possibility of interaction with neighboring galaxies.