The galaxy presents with a somewhat elongated morphology, though not highly cigar-shaped. The central region exhibits a high degree of smoothness and a bright, concentrated core. There is faint evidence of a disk-like structure surrounding the central region; however, this disk is not well-defined. The light distribution within the galaxy suggests some signs of past or ongoing interactions or mergers due to asymmetry and disturbances in its overall shape, where the central core is noticeably brighter than the outer disk. It appears the galaxy has a moderate mass and weak to moderate star forming activity. The overall color is towards the bluer end, which means it could host some younger stars.
