The galaxy presents as an elliptical morphology, with a smooth, concentrated central bulge exhibiting a yellow-orange hue, suggesting an older stellar population.  The isophotes are generally rounded. There is faint suggestion of a flattened disk component oriented roughly horizontally through the image, and hints of spiral arm structure, although the features are diffuse and lacking high definition.  The outer regions of the galaxy exhibit a significant decrease in surface brightness. Faint tidal disturbances appear minor, suggesting a previous minor interaction. The galaxy lacks any obvious strong dust lanes or active star-forming regions within the central region. Color gradients indicate a bluer halo or a less pronounced, outer disk component.
