The galaxy presents with a centrally concentrated morphology. The light is dominated by a smooth, somewhat rounded profile, but not perfectly circular. There is evidence of a faint, disklike structure. The colors are bluer in the central region, suggesting a concentration of younger stars or active star formation. The outer regions show a shift towards redder colors. There is potential evidence for a minor disturbance or possible interaction with another galaxy, seen in the slight asymmetry in the outer regions. It is not currently undergoing a major merger.