The galaxy presents a generally smooth and rounded morphology. The light distribution suggests an elliptical or lenticular galaxy type due to the lack of discernible spiral arms or a prominent disk structure. The central region exhibits a high degree of concentration, appearing bright and somewhat yellow in color, likely indicating an older stellar population. The outer regions of the galaxy gradually fade in intensity, forming a diffuse halo. There is no evidence of significant dust lanes or active star formation regions visible in the image. The overall appearance is consistent with a galaxy that has undergone substantial evolution and is now dominated by older stars. There does not appear to be any signs of major disturbances or recent mergers affecting the galaxy's structure. The object shows a distinct but not cigar shaped profile.
