The galaxy presents a generally smooth and elliptical morphology. The core region exhibits a concentrated luminosity, appearing bright yellow, indicative of an older stellar population. A fainter, bluer, and extended disk structure surrounds the central bulge, suggesting ongoing or recent star formation in the outer regions. The disk appears relatively undisturbed, lacking strong evidence of major mergers or tidal interactions. The axial ratio suggests a slightly elongated shape, but it is closer to round, with only a moderate degree of ellipticity. There is some indication of possible minor disturbances in the disk, but no clear signs of major merging activity.
