The galaxy appears as a centrally concentrated object, displaying a largely smooth morphology. There may be some faint signs of a disk structure within its outer regions. Its overall shape seems somewhat round. There are no major signs of on-going or recent merger activity. The galaxy shows a color gradient, appearing somewhat bluer in the central region and gradually becoming redder toward the edges. This color gradient potentially indicates a relatively young stellar population in the core and/or greater dust extinction in the outer regions.
