The galaxy presents as an elliptical or lenticular type, with a smooth, centralized light distribution. The core is bright, exhibiting a yellowish-white hue, suggesting an older stellar population. Moving outwards from the core, the color transitions to a greenish-yellow, possibly indicating a mix of older stars and some ongoing, low-level star formation. The outer regions fade into a dimmer, bluish haze, potentially showing the presence of a younger stellar population or dust. The galaxy appears relatively undisturbed, showing no signs of major mergers or tidal disruptions. Its overall shape is elongated, with a major axis approximately twice the length of its minor axis.
