The galaxy presents as a luminous, relatively smooth and rounded object. There is some evidence of a disk-like structure, but the dominant impression is one of spheroidal symmetry. The color profile suggests an evolved stellar population, with a significant fraction of stars nearing the red giant branch. There appears to be some minor internal disruption of the galaxy structure. Star formation is ongoing, but at a low rate. The galaxy exhibits a moderately high mass with relatively strong star formation. It's not currently involved in any major mergers.
