The galaxy presents as a centrally concentrated object with a smooth light profile. It exhibits a slightly elliptical shape, appearing more elongated than perfectly circular. The central region displays a bright, concentrated core. The color is generally yellowish-white, indicative of a population of older stars, though there are hints of bluer hues within the outer regions, potentially indicating some ongoing, though not necessarily dominant, star formation. There is no distinct spiral arm structure visible, nor is there evidence of a prominent dust lane. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal disruptions. Faint wisps of light extend beyond the central bulge, suggesting a more extended halo or disk component.
