The galaxy presents as a relatively smooth, elongated structure. It displays a centrally concentrated bulge, exhibiting a yellow-red hue. This core region appears to gradually fade out to the more diffuse edges. The overall shape is reminiscent of a lenticular galaxy, viewed at a significant angle to our line of sight. There is little evidence of spiral arm structure, however. The lack of distinct features suggests that the galaxy may be composed primarily of older stellar populations.
