The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The color profile exhibits a yellowish-white core, suggesting a population of older stars. The outer regions show a gradual color gradient towards a bluer hue, potentially indicating the presence of a younger stellar population within an extended disk. The galaxy lacks any prominent spiral arm structures or distinct dust lanes. Overall, the galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions.
