The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a spheroid-dominated morphology, likely an elliptical or lenticular galaxy, with little evidence of spiral arm structures. There is a distinct color gradient; the central region exhibits a yellowish hue, which transitions to a redder color in the outer regions. This color gradient might indicate a change in stellar population, with older, redder stars dominating the outer regions and a population of younger, slightly bluer stars concentrated towards the center. The overall roundness of the galaxy is apparent, with no significant distortions suggesting major mergers or tidal interactions. The outer edges appear diffuse and lack any sharp definition.
