The galaxy appears as a relatively smooth, centralized object. It exhibits a somewhat elliptical morphology, with a moderate degree of roundness. There is a slight hint of a disk-like structure, but the light is mostly concentrated towards the center. 

The color profile suggests a mixture of stellar populations. The core region displays a bluer hue, potentially indicative of younger, hotter stars or ongoing star formation. The outer regions appear redder, which may be due to a population of older stars or the presence of dust. There does not seem to be strong signs of active merging or major disturbances, although a subtle asymmetry is visible. Overall, this galaxy seems to be an intermediate mass galaxy with a relatively low rate of star formation.
