The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated, exhibiting a gradual decrease in surface brightness from the core outwards. The core region appears predominantly white, possibly indicating a population of older stars and/or a significant contribution from an active galactic nucleus. There is a slight color gradient observed towards the outer regions, shifting towards a more reddish hue, which could be indicative of a different stellar population or dust obscuration. A faint disk-like structure is possibly present. No strong spiral arm features or significant dust lanes are readily apparent. Based on the morphological characteristics, this galaxy is likely a relatively massive system with a moderate rate of star formation. There may be minor disturbances due to a potential merger. The overall structure suggests a dynamically relaxed system, potentially an elliptical galaxy undergoing passive evolution.
