The galaxy appears as a smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light distribution is relatively uniform, with a gradual decrease in intensity from the core outwards. There is no readily apparent spiral arm structure or significant dust lane obscuration. The color is predominantly yellowish-orange, suggesting an older stellar population and a relatively low rate of ongoing star formation. The galaxy's shape is neither perfectly spherical nor highly elongated, appearing moderately elliptical. No signs of major mergers or tidal disturbances are obvious, though a very slight asymmetry is present.
