The galaxy presents as a relatively smooth, centrally concentrated system. There appears to be a bright, yellowish core region which is likely a galactic bulge. The isophotes of the galaxy are generally elliptical. There is a slight color gradient, with the central region appearing yellower than the outer regions. The galaxy shows little evidence of spiral arm structure or significant dust lanes. Faint wisps of diffuse light extend from the core, contributing to a halo-like structure surrounding the brighter central region. There is no clear evidence of ongoing major mergers or tidal disturbances based on the smoothness of the features. The galaxy seems to be an elliptical or lenticular type system, with a mostly uniform structure.
