The galaxy presents as a somewhat elliptical, concentrated object with a smooth appearance. The central region exhibits a brighter, more intense luminosity, suggesting a dense concentration of stars or potentially an active galactic nucleus. There is a slight elongation and a gradual decrease in surface brightness extending outwards from the core. Colors are subdued, with a hint of redder hues concentrated toward the central bulge. Subtle bluer tones are visible in the outer regions, possibly indicating some ongoing star formation but the overall morphology suggests that star formation is relatively low. The galaxy displays no obvious spiral arm structure or significant tidal disturbances. There is a slight irregularity in the light distribution with the east side appearing less bright than the west. The galaxy is relatively isolated, appearing without any obvious merging partners or close companions.
