The galaxy presents a largely smooth, elliptical morphology, exhibiting a high degree of radial symmetry. Its core region is characterized by a concentration of luminosity, possibly indicating a high stellar density. The central light is slightly redder in appearance than the surrounding area. Moving outward from the core, the luminosity gradually decreases with no obvious spiral arm structures visible. There is little indication of significant tidal disturbances or ongoing major mergers, with no distinct tails or bridges of stellar material detected, though there may be minor disturbances in the outer halo. It does not exhibit a highly flattened disk-like structure; it is relatively round. Star formation is likely low.