The galaxy presents as a centrally concentrated spheroid with a smooth luminosity profile, suggesting an elliptical morphology or a lenticular galaxy seen face-on. The core is bright and appears yellowish-white, indicative of an older stellar population. A subtle color gradient is observed moving outward from the core, transitioning to a slightly bluer hue. This may reflect a small degree of on-going star formation. There is no readily observable spiral arm structure or significant dust lane features present. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or major mergers. A slight elongation is perceptible, suggesting it is not perfectly spherical but rather a spheroid with an intermediate shape. The size is small but within the typical range.