The galaxy appears as a centrally concentrated, somewhat diffuse object. It exhibits a relatively smooth morphology with a dominant spheroidal component. There is a subtle color gradient observed, with a bluer hue toward the center which is indicative of younger stellar populations or active galactic nuclei activity. The galaxy is mostly round in shape, but it has a very slight distortion to it. There is no clear evidence of strong spiral arm structures or a well-defined disk. The lack of prominent dust lanes further supports the classification of a relatively early-type galaxy. No other galaxies are seen to be merging with this galaxy.
