The galaxy presents as a relatively smooth, elliptical-like structure with a slight elongation. The core exhibits a concentrated, bright luminosity, indicative of a significant stellar density. A subtle gradient of color is observed, with the central region appearing yellower, transitioning to a bluer hue in the outer regions. This color gradient may suggest variations in stellar populations, with older stars dominating the core and younger, hotter stars present in the surrounding area. Possible minor disturbances are observed in the overall shape. Despite the smoothness, there seems to be some interaction with the object on its right side. This warrants further inspection and comparison with other data.
