The galaxy presents a generally smooth morphology, with a dominant central bulge. The overall shape appears to be somewhat elliptical, though not perfectly round. There may be a faint disk structure present, but it is not readily apparent in the image, possibly due to the viewing angle or internal dust obscuration. The color is notably yellow/orange in the central region, possibly indicating an older stellar population and less active star formation in that area. Fainter, bluer regions may be present at the outer edges, hinting at some ongoing star formation. There are possible signs of minor disturbances in the morphology, potentially indicating a past or ongoing interaction or merger.