The galaxy appears to be a relatively smooth object, exhibiting a concentrated central bulge. The overall color suggests a population of older stars. There is a very subtle hint of a disk structure. The galaxy presents an elliptical-like morphology, with a slight elongation. There appears to be little to no evidence of ongoing major star formation. The galaxy does not seem to be strongly interacting with other galaxies, and overall, the structure appears relatively undisturbed.
