The galaxy presents as a primarily smooth, elliptical-like structure. There appears to be a bright, concentrated central bulge, transitioning into a slightly fainter halo. The overall color is a yellowish hue in the inner region, suggestive of an older stellar population, with a slight shift towards redder tones. The outer regions exhibit a faint greenish color, which could be due to younger stars. There is little evidence of defined spiral arms or significant dust lanes. The overall form appears largely undisturbed, without signs of ongoing major mergers or tidal disruptions.
