The galaxy exhibits an elliptical morphology, appearing largely smooth and well-defined. The light distribution is centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. There is a slight elongation to the galaxy's shape; it is observed to be moderately flattened, rather than perfectly spherical. No distinct features such as spiral arms or prominent dust lanes are readily apparent. The galaxy's color is generally redder, suggesting a stellar population dominated by older stars and potentially a lower rate of ongoing star formation. There is no evidence of recent or ongoing major merger events. The galaxy's overall structure indicates that it's a large, somewhat massive elliptical galaxy.