The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge. There is minimal visual evidence of spiral arms or distinct disk features. The light distribution appears largely uniform, with a gradual decrease in intensity from the core outwards, suggesting an older stellar population. There are no obvious signs of active star formation regions or dust lanes. The overall color profile is yellowish, consistent with a galaxy dominated by older, redder stars. The galaxy's shape is generally round, showing no significant elongation or distortion. There are no indications of tidal tails, mergers, or major disturbances in its morphology.
