The galaxy appears to be a relatively smooth, elliptical-like structure. Its overall shape is more elongated than circular, though not cigar-shaped. The light distribution suggests a concentrated central bulge with a gradual decrease in brightness outward, lacking distinct spiral arm features. There is a slight asymmetry in the outer regions but no obvious signs of major disturbances or ongoing merging activity. The galaxy appears to be relatively quiescent with low star forming properties.
