The galaxy presents as an elliptical-like structure, exhibiting a smooth, centrally concentrated morphology. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features usually associated with disk galaxies. The core region is noticeably brighter and exhibits a yellow hue, suggestive of an older stellar population. The galaxy has a fairly circular shape with only a small amount of distortion, with some slight asymmetry. There are no obvious signs of recent or ongoing major merger events. The extended halo surrounding the core gradually fades into the background, suggesting a diffuse distribution of stars.
