The galaxy presents as a slightly elongated, diffuse structure with a relatively smooth overall appearance. Its central region exhibits a bright, concentrated core, suggestive of a significant stellar population or active galactic nucleus. Moving outwards from the core, the light gradually diminishes, indicating a decrease in stellar density. There is some evidence of a disk-like structure, although it's not sharply defined. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, although minor disturbances may be present. There is a hint of bluer colors in the outer regions, which could indicate ongoing star formation. The overall morphology leans toward an early-type spiral or lenticular galaxy, but could also simply be a galaxy with a large central bulge and very weak spiral arms.
