The galaxy presents a largely smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density or an active galactic nucleus, though without spectroscopic data, the presence of an AGN cannot be confirmed. The overall color profile appears relatively red, hinting at an older stellar population with lower levels of ongoing star formation. The galaxy displays a generally rounded shape. There is some visual evidence of a potential minor disturbance. The structure of the galaxy is distorted, suggesting a recent or ongoing interaction with another galaxy.
