The galaxy appears as a fairly smooth and centrally concentrated object, generally elliptical in shape. The color profile suggests a relatively older stellar population, with the core exhibiting a bluer hue. Fainter, diffuse light extends outward from the core, with slight elongation, however no prominent spiral arms or bar features are discernible. There is some evidence of possible minor disturbances or asymmetry in the outer regions, possibly indicative of past or ongoing interactions. Overall, the galaxy seems to be a spheroid with a moderate redshift.
