The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears elliptical, exhibiting a high degree of roundness. There is a bright, yellowish core that gradually fades into a diffuse halo. No distinct spiral arms or prominent dust lanes are discernible. The galaxy's color suggests a population dominated by older stars, with a relatively low rate of current star formation. There are no obvious signs of recent or ongoing major mergers or significant tidal disturbances. The overall structure suggests an evolved system, consistent with an elliptical classification.
