The galaxy presents as a single, relatively smooth, concentrated object. It has an elliptical appearance, close to round in shape, with a noticeable central bulge that gradually diffuses outwards. The core exhibits a high degree of luminosity, suggesting a concentration of older stellar populations or possible AGN activity. There appears to be no strong evidence of spiral arms or distinct morphological features beyond the general elliptical profile. The light profile appears consistent with an early-type galaxy, likely a lenticular or elliptical galaxy. There are very slight color variations within the galaxy; these variations are subtle, but might be related to differences in stellar populations.
