This galaxy presents as a moderately luminous system, appearing largely elliptical in shape but potentially exhibiting some disk-like features. The central bulge is bright and concentrated, suggesting a high stellar density. The galaxy's overall color appears yellowish-white, indicating a significant population of older stars and/or substantial dust obscuration. There is a noticeable extension of the galaxy's light along a slightly elongated axis. A fainter companion galaxy is visible in close proximity, potentially gravitationally interacting with the main galaxy. The system may be in an early stage of a minor merger, indicated by some subtle distortions in the primary galaxy's overall structure. There is a slight color variation in the fainter regions of the galaxy, hinting at localized star formation or differential dust extinction, though overall the color is relatively uniform.
