The galaxy presents as a primarily smooth, elliptical morphology. The light distribution suggests a centrally concentrated spheroid, with a gradual decrease in luminosity outward from the core. The overall color appears somewhat red. There may be a very faint, diffuse disk surrounding the central bulge. No distinct spiral arm structures or prominent dust lanes are visible. The general appearance of the galaxy indicates it may be a relatively evolved system, likely with lower rates of star formation. There appears to be no evidence of tidal interactions or ongoing mergers. It displays a generally undisturbed and symmetric structure.
