The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally condensed, gradually decreasing in intensity outwards. The galaxy exhibits a subtle elongation, deviating slightly from a perfect circular form. There is minimal evidence of spiral arms or significant disk-like features. Its overall color appears redder, suggesting a population of older stars, and a lower rate of active star formation. There is no obvious dust lane or distinct substructure evident in the image, the galaxy appears as an evolved system.
