The galaxy presents as a relatively smooth, elliptical morphology, appearing somewhat rounded in shape. There is a possible very slight disturbance or faint arm structure visible, but it is not a highly pronounced feature. The galaxy exhibits a color gradient, appearing more yellow-red in the central region and bluer on the edges, which could indicate a difference in stellar population density, and possibly ongoing star formation, particularly at the edges. The redder colors are indicative of older stars towards the center of the galaxy, while blue colors at the edges indicate younger stars are forming. Overall, the galaxy appears to be relatively isolated with no signs of major mergers in the recent past.
