The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. A prominent bulge dominates the core, showing a yellowish-orange hue indicative of an older stellar population. Fainter, diffuse extensions surround the central bulge, lacking defined spiral arm structures. The overall shape tends towards rounded rather than elongated, with a slight disk-like appearance. There are indications of a potential tidal disturbance or recent merger event, with subtle asymmetries and faint plumes extending from the main body of the galaxy. Areas of blue-ish light are observed in the main disk and the surrounding plumes and disturbances, hinting at some recent star formation.
