The galaxy presents as a relatively smooth, elliptical-like structure with an apparent intermediate axial ratio. A bright central bulge is readily apparent, suggesting a significant concentration of stars toward the galactic nucleus. The overall color appears to be slightly redder in the central regions, possibly indicative of an older stellar population, while the outer regions exhibit a bluer tinge, potentially indicating more recent star formation. There is a subtle hint of a disk structure; it appears to be undergoing minor disturbances. Given its morphology and color distribution, this galaxy is likely a relatively massive system with a moderate star formation rate.
