The galaxy presents as an elliptical morphology. A centrally concentrated bulge is visible, exhibiting a yellowish-white hue, indicative of an older stellar population. There is little evidence of spiral arm structure, with a smooth light distribution overall. The galaxy is relatively compact in size. The overall color suggests a relatively low rate of ongoing star formation. Minor, subtle distortions are observed in the galaxy's outer isophotes, though no major merger events are apparent in the image. The overall impression is that of a relatively massive, evolved galaxy with a suppressed star formation rate and possible minor interactions.
