The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The galaxy exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. Color gradients are visible, with the central bulge displaying a yellowish hue, suggestive of an older stellar population. The outer regions exhibit a bluer tint indicating the presence of some younger stars, although less prominent than the central population. There appears to be no noticeable spiral arm structure or significant dust lanes. There are no signs of ongoing mergers or tidal disturbances visible in this image. The galaxy presents an appearance of relative morphological quiescence.
