The galaxy presents a smooth, largely featureless morphology. It exhibits a concentrated central bulge region, yellowish-white in color, indicative of an older stellar population. The overall shape appears nearly circular with an absence of spiral arm structures or significant disturbances. Faint, diffuse light extends outwards from the central region, gradually fading into the background sky. The galaxy appears relatively isolated with no obvious signs of tidal interactions or recent mergers visible in this image. Its color gradient suggests possible radial variations in stellar population or dust content. Based on morphology, it is consistent with an elliptical galaxy.
