The galaxy appears to be a relatively smooth, elliptical system, exhibiting a centrally concentrated light profile. It displays a slightly elongated morphology, appearing more 'in between' round and cigar shaped, but not exhibiting a clear disk structure. There is a hint of some minor internal structure or disturbance. The galaxy's color suggests a population dominated by older stars, emitting strongly in the redder bands, while the presence of some bluer light indicates the possibility of some ongoing, but limited star formation.
