The galaxy presents a primarily smooth morphology with a notable central bulge. The overall shape appears elliptical, exhibiting a slight elongation. The central region is bright and concentrated, suggesting a high stellar density. The outer regions display a gradual decrease in luminosity, forming a diffuse halo. There's a hint of a disk-like structure, though it is not clearly defined. No distinct spiral arms or bar structures are discernible. The color profile suggests a mature stellar population, dominated by older, redder stars, particularly within the central bulge. There are faint signs of possible minor disturbances.
