The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a concentrated central bulge that dominates its overall structure. The light distribution is highly centrally peaked, with a gradual decrease in intensity towards the outer regions. There is little evidence of spiral arm structure or significant dust lanes; however, there is some subtle, irregular light distribution to the left, hinting at possible minor disturbance or interaction. The galaxy's color is generally yellowish to reddish, suggesting a population of older stars with a lower rate of ongoing star formation. It appears nearly circular.
