The galaxy appears to be an elliptical or lenticular type. It presents as a generally smooth, centrally concentrated object. The light profile indicates a relatively featureless morphology, with a high degree of radial symmetry, suggestive of an older stellar population. There is little evidence of spiral arms or significant dust lanes. A subtle color gradient may indicate a variation in stellar populations across the galaxy, with a slightly bluer hue in the outer regions, hinting at some recent star formation, or the presence of a younger stellar population in the surrounding halo. The overall round appearance further reinforces its classification as an elliptical galaxy.
