The galaxy exhibits a generally smooth morphology, with a centrally concentrated luminosity profile. The light distribution appears largely spheroidal, with a high degree of circular symmetry. There is a subtle color gradient, with the central region displaying a yellowish-white hue, potentially indicative of an older stellar population. The outer regions appear fainter and slightly redder. There is no clear evidence of spiral arm structure or a prominent disk component from this angle. The galaxy is relatively undisturbed, showing no signs of major mergers or significant tidal interactions. Minor disturbances or the presence of a faint, unresolved disk cannot be ruled out.
