The galaxy presents as a predominantly smooth, elliptical morphology. It appears relatively round, with minimal discernible features suggestive of spiral arms or a distinct disk structure. The central region exhibits a high degree of luminosity, indicative of a significant concentration of stars. The light intensity gradually diminishes towards the outer edges, with no obvious irregularities or signs of ongoing major mergers, though some minor disturbances cannot be ruled out. The galaxy's overall color appears slightly red-shifted, suggesting a moderate distance and indicative of an older stellar population.
