The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a roughly elliptical morphology, appearing somewhat rounded in shape. There is a noticeable color gradient, with the central region displaying a yellowish-white hue, suggesting a population of older stars. The outer regions appear fainter and slightly redder, potentially indicating a lower density of stars or the presence of dust. No distinct spiral arms or bar structures are discernible. There's no clear evidence of any ongoing major mergers or significant tidal disturbances. The galaxy appears relatively isolated, with no obvious interacting companions nearby within this field of view.
