The galaxy presents as a largely elliptical structure, exhibiting a smooth, symmetrical light distribution with minimal discernible features such as spiral arms or a prominent central bar. The core of the galaxy appears bright and concentrated, suggestive of a dense stellar population or an active galactic nucleus, though the image resolution limits conclusive assessment. The galaxy gradually fades into the surrounding space. No signs of tidal tails or major disturbances are present, indicating that the galaxy is likely not undergoing a major merger. The color profile indicates a population of older stars dominating the galaxy.
