The galaxy presents a generally smooth and rounded morphology. There is a bright central bulge with a somewhat diffuse appearance. The color index indicates a redder overall color, suggestive of an older stellar population, but with some possible subtle blue regions. The galaxy appears relatively isolated, with no immediately obvious major merging features. There is evidence of some slight distortion. It may have a spiral shape, however this is not easily determined due to the resolution of this image. The galaxy is a substantial presence within the frame, indicating considerable luminosity and mass.
