The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards. The overall color appears to be trending towards the redder end of the spectrum, suggesting an older stellar population with diminished star formation. There is some evidence of a disk-like structure, though faint and not well defined. There does not appear to be any evidence of major tidal disturbances or ongoing mergers. The galaxy appears fairly isolated and undisturbed.
