The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy. Its light profile suggests minimal internal structure, lacking prominent spiral arms or a distinct bar. The central bulge is bright and concentrated, fading outwards into a more diffuse halo. The galaxy appears to be fairly rounded in shape. There is a slight hint of color variation within the galaxy, with the central region showing a yellower hue, possibly indicating an older stellar population. Star formation is low, based on the lack of blue color. There is no clear evidence of ongoing mergers or tidal interactions, with no apparent distortions or debris tails.
