The galaxy presents a generally elliptical morphology. It exhibits a smooth, centralized concentration of light, indicative of an older stellar population. The core region is the brightest, gradually fading into the outer regions. The galaxy has a slight disc-like appearance, but is primarily smooth and elliptical in shape. There is a suggestion of a slight tidal disturbance, but it is not substantial. The light from the galaxy exhibits a spectral gradient, with bluer hues emanating from the outer regions and redder tones dominating the central bulge. It seems to be a well-formed, stable galaxy, and appears relatively isolated, without evidence of a major ongoing merger.
