The galaxy presents a largely smooth, elliptical morphology. A bright, concentrated central bulge is evident, surrounded by a more diffuse halo. The galaxy exhibits a yellowish hue in its central region, transitioning to a redder color towards the outer edges of the halo. The lack of readily visible spiral arms or significant dust lanes suggests a relatively evolved system. There is no clear evidence of ongoing major mergers or tidal distortions, though subtle asymmetries cannot be entirely ruled out given the image quality. The overall appearance indicates a population of older stars, consistent with the colors and morphology observed.
