The galaxy presents as a relatively compact, elliptical or lenticular structure, displaying a smooth, somewhat featureless morphology. It is roughly circular in appearance, with a bright, concentrated core region that gradually diffuses outward. The light profile suggests minimal to no spiral arm structure or prominent dust lanes. The color gradient shows a central yellowish-white hue, possibly indicating an older stellar population. The overall impression is that of a quiescent system, with limited ongoing star formation. There is no visual evidence of significant tidal disturbances or recent merger activity, suggesting it is a relatively isolated galaxy.
