This galaxy presents an elliptical morphology, exhibiting a smooth, diffuse distribution of light. The central bulge is prominent, displaying a concentrated luminosity gradient. The overall color is consistent with an older stellar population. The galaxy has a relatively high spheroidal component. There is some evidence of disturbance in the disk, but the nature of this is not clear. The overall light distribution appears to be concentrated toward the center, with a fairly regular, symmetric profile. The dust distribution appears low, or generally unobservable in this image.
