The galaxy presents a generally smooth, rounded morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity outward from the core. There is a slight elongation, but it is mostly circular. The color profile indicates a dominant population of older stars, with the light trending towards the redder end of the spectrum. Little evidence of spiral arms or active star formation is present in this image, suggesting it is an older galaxy with low star formation rate and a high mass. The galaxy appears relatively undisturbed.
