The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a somewhat round morphology. There is no apparent bulge or spiral arm structure, suggesting a lack of ongoing active star formation. The galaxy shows a redder hue centrally, fading into more green and blue hues at the edges, which indicates a possible transition in stellar population from older stars toward the center, towards younger stars toward the edges, as well as potential dust reddening towards the center. Overall, the galaxy seems relatively undisturbed, with no signs of major mergers or tidal disturbances.
