The galaxy presents as a relatively compact, smooth structure. Its overall color is dominated by redder wavelengths, with some evidence of a subtle blue component, indicating the presence of both older stellar populations and regions of ongoing star formation. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is no strong indication of spiral arms or a distinct disk structure. There is no obvious ongoing major merger. The overall morphology appears to be elliptical, with a very slight degree of ellipticity that makes it almost circular.
