The galaxy appears to be a relatively smooth, early-type system, likely an elliptical or lenticular galaxy. It exhibits a centrally concentrated luminosity profile with a gradual decrease in surface brightness outward. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's color is generally red, suggesting an older stellar population and a low rate of ongoing star formation. It appears nearly round in projection with a slight indication of ellipticity. There might be minor distortions in the outer regions indicating possible past interactions, but overall, the galaxy appears relatively undisturbed.
