The galaxy presents as a relatively compact object, approximately elliptical in shape, with a noticeable central bulge. The core exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially an active galactic nucleus. Moving outwards from the core, the intensity of light diminishes, forming a halo-like structure that appears slightly elongated.

There is a subtle irregularity in the galaxy's overall form, hinting at possible tidal interactions or previous minor merger events. A faint distortion is observed on one side of the galaxy, indicating a potential disturbance in its gravitational equilibrium. The color profile suggests an older stellar population, with a generally redder hue dominating the galaxy's overall light emission. Faint traces of bluer light may indicate some ongoing star formation, albeit at a low rate.
