The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a subtle ellipticity, tending toward a rounded shape, but not perfectly circular. The central region exhibits a bright, concentrated luminosity, transitioning to a fainter, more diffuse halo surrounding it. There is minimal indication of spiral arm structure or distinct features within the disk. The color profile suggests an older stellar population, with a yellow-orange hue dominating the central region. There appears to be no evidence of major ongoing mergers or significant tidal disturbances. Subtle irregularities in the outer regions might suggest minor disturbances, though these are not strongly pronounced.
