The galaxy exhibits an overall morphology that appears relatively smooth, though not perfectly so. A bright, concentrated central region dominates the galaxy's structure, suggesting the presence of a significant bulge or core. This central region appears nearly spherical.

Surrounding the core is a fainter, somewhat diffuse halo of light. This halo is not uniformly distributed. There are suggestions of slightly irregular features, such as distortions or faint tidal tails, indicating potential interactions or past mergers. The distribution of light in the outer regions is not uniform or symmetric, exhibiting a subtle irregularity. 

The color gradients across the galaxy suggest variations in stellar populations. The central region shows a bluer hue, potentially indicative of younger, hotter stars or active star formation. The outer regions appear somewhat redder, which could be attributed to older, cooler stellar populations.
