The galaxy appears as a moderately luminous, elliptical-shaped object with a fairly smooth texture and profile. The light distribution suggests a concentrated central bulge, indicated by a yellowish core. The overall color suggests a population of older stars, with minimal discernible dust lanes or active star forming regions based on the lack of intense blue light. The elongation of the galaxy is moderate, neither perfectly spherical nor overly flattened. There is some evidence of minor asymmetry or disturbances in the outer regions, possibly indicative of past interactions, but not conclusive. Overall, the galaxy presents as an intermediate elliptical, likely relatively massive, with ongoing but quiescent stellar formation, exhibiting primarily older stellar populations.
