The galaxy presents as a centrally concentrated, elliptical-like system. The light distribution appears relatively smooth and diffuse, lacking any distinct spiral arm features or a prominent bar structure. The core exhibits a bright, concentrated luminosity, suggesting a substantial stellar population or potentially an active galactic nucleus. The galaxy's overall color appears to be redder, indicating an older stellar population, consistent with an elliptical morphology. There is a slight elongation in the shape of the galaxy, deviating from a perfectly circular profile. No significant dust lanes or regions of active star formation are readily apparent.
