The galaxy presents as a largely featureless, elliptical-shaped object with a concentrated central bulge that displays a yellowish hue, indicating a population of older stars. The outer regions of the galaxy appear more diffuse and reddened, further suggesting an aging stellar population. There is a subtle transition in color and intensity from the core to the outskirts, without any obvious spiral arms or distinct features. The smoothness and lack of prominent structures implies a relatively quiescent star formation rate. Overall, the galaxy is a fairly rounded structure and there is no sign of any ongoing major interactions with other galaxies, such as tidal tails or strong morphological disturbances. The light profile suggests the galaxy is relatively isolated.