The galaxy presents as a single, centrally concentrated luminous object with a smoothly distributed light profile. The overall shape appears largely elliptical, exhibiting a high degree of roundness with a slight deviation towards a more intermediate form. There is no visually discernible evidence of spiral arms or a galactic disk. The galaxy displays a dominant yellowish hue, suggesting a population of older stars. The smooth light distribution indicates little to no ongoing major star formation. There are no apparent signs of significant tidal disturbances, merging activity, or close companions that would indicate recent or ongoing interactions with other galaxies. Overall, the galaxy’s appearance is consistent with that of an early-type galaxy characterized by an older stellar population and a smooth, featureless structure.
