The galaxy presents a generally smooth morphology. The central region is bright and concentrated, suggesting the presence of a bulge. The overall shape of the galaxy appears to be somewhere in between round and elliptical. There is no clear evidence of spiral arms or a distinct disk structure. Faint features are present with what appears to be slight disturbances or irregularities in its outer regions, but no clear sign of ongoing major mergers. Overall, the galaxy appears relatively undisturbed and quiescent. The blueness could be due to intermediate star formation.
