The galaxy presents as a relatively compact object with a central bulge exhibiting a diffuse, hazy appearance. Its overall color profile suggests a combination of stellar populations. The core region appears predominantly white, indicative of older, more evolved stars. Emanating outward from the core is a bluish halo, suggesting the presence of ongoing or recent star formation. There appear to be some features in the disk, but it is difficult to tell if they are the result of a galactic merger. The morphology isn't particularly smooth. The galaxy may be undergoing a minor interaction, or it could be that the image is simply not detailed enough to draw conclusions.
