The galaxy presents as a relatively smooth, centrally concentrated object. It is characterized by a dominant spheroidal component, appearing nearly round in projection. The core exhibits a yellowish hue, possibly indicating an older stellar population. A less distinct, diffuse bluish halo surrounds the core, potentially suggesting some ongoing or recent star formation activity, although at a low rate. There are some hints of minor disturbances in the outer regions, which may suggest past or ongoing interactions with other galaxies. Overall, the galaxy appears to be a relatively massive system, with no clear signs of a prominent disk structure.
