The galaxy presents as a roughly elliptical object with a concentrated central bulge. The core region exhibits a bright, high-intensity glow, indicating potentially high stellar density or active galactic nucleus activity. Surrounding the core is a diffuse, somewhat amorphous structure, possibly indicative of a disk component, although distinct spiral arm features are not clearly visible. The overall color profile suggests a mix of stellar populations, with the central bulge appearing more yellowish, indicating older, redder stars, while the outer regions show a slight bluer hue, hinting at the presence of younger, hotter stars or ongoing star formation. There is also a slightly perturbed morphology with a small distortion on one side of the galaxy.
