The galaxy presents as a single, fairly symmetrical, smooth, and rounded object. It exhibits a concentrated central bulge, which appears yellow-white, suggesting a population of older stars. The color shifts toward red in the central region, indicative of a more aged stellar population.

Moving outward from the core, the surrounding galactic structure gradually fades, appearing to transition into a less luminous halo or disk. The outer regions show a subtle gradient in color, becoming slightly bluer, which is consistent with the presence of a younger stellar population contributing to ongoing, although low, star formation. 

There are no apparent signs of spiral arms or other disk features, nor any evidence of ongoing mergers or tidal interactions. The galaxy appears relatively undisturbed, with no major distortions in its overall shape.
