The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth appearance with no readily discernible spiral arms or bar structure. The color is predominantly yellow, suggesting an older stellar population with fewer young, blue stars. The galaxy appears generally rounded in shape, with a slight elongation. There is no evidence of a major ongoing merger, although there are minor distortions to the galaxy's morphology indicating possible interaction with other nearby systems. The galaxy’s size is fairly compact, and the light is concentrated in the central regions.
