The galaxy presents a roughly elliptical morphology, with a bright, concentrated central bulge. The color of the bulge is predominantly yellow-white, suggesting an older stellar population. Fainter, bluer light extends outward from the bulge, indicating the presence of a disk component. The disk appears relatively smooth with hints of spiral structure. There is a small, diffuse red region slightly offset from the nucleus, indicating a region of either dust extinction or ionized gas. The overall structure suggests a possible classification between an elliptical and a spiral galaxy, likely leaning towards a lenticular classification with intermediate mass. There is no definitive evidence of a recent major merger, though there may be minor disturbances in the disk.
