The galaxy presents as a moderately luminous, elliptical-like structure. It appears to be somewhat smooth and centrally concentrated, with a yellowish core indicative of older stellar populations. There are no apparent spiral arms or prominent dust lanes. The isophotes seem more round than cigar-shaped, extending into a faint halo that gradually fades into the background. There appears to be a minor disturbance on the left side of the galaxy, where a bluish formation may be present. This could indicate a potential interaction or minor merger event. The overall color profile suggests a relatively quiescent galaxy with little ongoing star formation in the main body, but potentially some activity around the blue formation.
