The galaxy presents as a centrally concentrated system with a spheroidal morphology. The core appears bright and yellowish, suggestive of an older stellar population. Fainter, bluer light extends outward from the central bulge in a somewhat disk-like structure. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly round nor highly elongated. There are hints of subtle disturbances in the outer regions, which could be indicative of minor interactions or past mergers. Overall, it is a galaxy with both smooth and featured aspects, indicating a complex history of formation and evolution. The light is more concentrated in the center, suggesting a higher density of stars in the central region.
