The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge region displaying a yellowish-orange hue, suggesting an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. The overall roundness of the galaxy is notable, with minimal deviation from a circular shape. There may be minor disturbances present in the galaxy's morphology which could indicate a weak tidal interaction or past minor merger event, visible as a slight asymmetry in the outer regions. The light from the galaxy indicates that there is suppressed star formation.
