The galaxy presents as a moderately compact, elliptical-like system. It has a generally smooth appearance with no strong visual indications of spiral arm structures or significant dust lanes. The overall light profile suggests a concentration of stellar density towards the center, with a gradual decrease in brightness towards the outer edges. Color gradients are subtle, the core showing a slightly yellower/redder hue compared to the bluer fringes of the galaxy, which may indicate an older stellar population dominating in the central regions. There is a very slight elongation of the galaxy, but it is close to being a spherical shape. The image suggests the galaxy is relatively isolated, with no visually apparent tidal disturbances or nearby companion galaxies that would indicate a recent or ongoing merger event. There are no major signs of any starburst.
