The galaxy appears to be elliptical, with a smooth, diffuse light distribution. It exhibits a roughly circular morphology with a high degree of central concentration. The galaxy is characterized by a dominant yellow-orange hue, indicative of an older stellar population. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy displays a relatively high degree of smoothness with very little indication of irregular features or ongoing merger activity. The light distribution seems to fade gradually towards the outer regions of the galaxy. The galaxy is isolated and appears to be non-interacting.
