The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge exhibiting a bright, yellowish-white hue, suggesting an older stellar population. The overall shape appears to be somewhat rounded, though not perfectly circular. A faint disk-like structure is subtly discernible, indicating the presence of some organized rotation. The outer regions of the galaxy fade into the background with decreasing surface brightness. There is no strong evidence of active star formation regions or prominent spiral arms. No obvious signs of major mergers or significant tidal disturbances are observed.
