The galaxy exhibits a predominantly smooth morphology, with a concentrated central bulge. Its overall shape is roughly elliptical, appearing somewhat rounded but trending towards an intermediate elongation. There's no readily apparent indication of spiral arm structures or strong disk features. Evidence suggests it is a galaxy which is not currently undergoing a major merging event. The color gradients indicate a population of older stars dominating the central regions, with bluer populations existing within the outer edges of the main body of the galaxy.