The galaxy presents as a relatively compact and luminous object. It exhibits a central bulge which is fairly bright. A faint disk structure appears to extend outwards from the bulge. The disk shows subtle features, potentially indicative of spiral arms or dust lanes, though these features are not sharply defined. There is a slightly uneven light distribution within the disk, and there are hints of possible disturbances within its structure. The overall color profile suggests a mix of stellar populations, with the central region appearing bluer than the outer regions. There appears to be ongoing or recent star formation activity, but likely at a moderate rate.
