The galaxy presents as a single, moderately bright object with an elliptical morphology. It exhibits a smooth light profile, lacking any distinct spiral arms or prominent dust lanes. The color appears relatively uniform across the galaxy, trending towards yellow-orange, suggesting an older stellar population with less ongoing star formation. There are no readily apparent signs of a major ongoing merger, although subtle disturbances in the outer regions cannot be entirely ruled out given the image resolution. The galaxy displays a somewhat rounded shape, deviating slightly from a perfect circle. Based on the observed color and morphology, this galaxy likely represents a relatively massive system that ceased vigorous star formation a significant amount of time ago.
