The galaxy presents as a relatively smooth, elliptical-like structure, appearing mostly round in projection. Its light profile is centrally concentrated, with a gradual decrease in surface brightness outwards. There's a noticeable color gradient, transitioning from a yellowish-white core to a slightly redder halo. No distinct spiral arms or prominent dust lanes are visible, and the galaxy appears undisturbed, with no signs of ongoing major mergers or significant tidal interactions. Based on its redder outer regions, we can assume there's a population of older stars. Star formation activity is likely subdued.
