The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish-white hue, potentially indicative of an older stellar population. There is a subtle elongation to the galaxy's shape; it does not appear perfectly spherical. Faint, diffuse extensions of light are observed around the central region, suggesting a gradual decrease in stellar density with increasing distance from the galactic center. There is no evident spiral arm structure or significant dust lane obscuration visible in this image. No major signs of disturbance such as tidal tails are present. The morphology appears relatively undisturbed and quiescent.
