The galaxy presents as a centrally concentrated, elliptical morphology with a smooth light distribution. The core region exhibits a bright, relatively homogenous luminosity profile with a yellowish-white hue, suggesting a population of older stars dominating the central mass. The light fades gradually outwards from the core, lacking any distinct spiral arm structures or prominent dust lanes. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances. The galaxy appears fairly isolated and undisturbed. Given the compact nature of the galaxy and color of the central bulge, it is likely a relatively massive system.
