The galaxy presents as a concentrated, elliptical-like structure with a smooth, fairly homogenous appearance. The core exhibits a bright, yellowish-white glow that gradually diffuses outwards. No distinct spiral arms or prominent dust lanes are discernible. The overall color profile suggests a relatively old stellar population, as indicated by the lack of strong blue emission typically associated with ongoing star formation. There is no obvious tidal debris or morphological disturbance, suggesting the galaxy is relatively isolated and unperturbed. The shape is mostly round, without significant elongation or asymmetry. No signs of active galactic nucleus activity are immediately apparent from the image.
