The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. Its color index suggests a population dominated by older stars, with minimal evidence of ongoing star formation. There is no visible spiral arm structure or significant dust lane obscuration. The galaxy exhibits a near-perfectly circular isophotal shape, displaying no obvious signs of tidal disturbances or interactions with companion galaxies. The overall impression is that of a relaxed and evolved system.
