The galaxy presents as a relatively compact, yellowish-orange structure, suggesting an evolved stellar population. Its morphology appears mostly smooth, with a discernible central concentration. There is a slight elongation, but overall it exhibits a rounded appearance. No distinct spiral arms or prominent dust lanes are visible. There appears to be some minor tidal features, possibly indicating a past or ongoing interaction or merger event, but the overall structure remains mostly undisturbed. The galaxy's color indicates relatively low star formation rate with a population dominated by older stars.
