The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core exhibits high luminosity, potentially indicative of an active galactic nucleus or a dense stellar population. The overall shape is close to circular, showing minimal evidence of a disk-like structure or significant irregularities. The color profile suggests the presence of older stellar populations, with a slightly redder hue observed towards the outer regions, while the center is bluer, which might be indicative of ongoing star formation. There are some minor disturbances noted in the immediate area. The galaxy does not appear to be undergoing a major merger, but small interactions in its past may have occured.
