The galaxy presents as a relatively smooth, elliptical structure with a prominent central bulge. The core exhibits a bright, concentrated luminosity, suggestive of a high stellar density or potentially an active galactic nucleus. Moving outward from the core, the light gradually diffuses, indicating a decreasing stellar population density. The galaxy has a slight elongation, leaning towards a flattened spheroidal shape rather than a perfect sphere. Faint hints of bluer regions are subtly visible around the periphery. A faint, distorted light is observable on the left side.
