The galaxy presents as a relatively smooth and elliptical structure. The light distribution appears concentrated towards the center, with a gradual decline in surface brightness moving outwards. It has a generally homogenous color profile, presenting a yellowish hue indicative of a population of older stars and a likely lower rate of current star formation. The galaxy is elongated, appearing more "in between" round and cigar shaped. No obvious spiral arms or significant dust lanes are visible. There are no indications of a major ongoing merger or significant tidal disturbances. There are signs of minor disturbances.
