The galaxy appears to be an elliptical or lenticular type. Its morphology exhibits a dominant smooth, centrally concentrated bulge. The overall light distribution is diffuse, with a centrally peaked brightness profile. There is a clear lack of defined spiral arms or significant dust lanes, suggesting a relatively quiescent star formation history. The color profile indicates a redder overall population, potentially dominated by older stars. The galaxy's shape is slightly elongated. No obvious signs of major mergers or tidal disturbances are apparent.
