The galaxy exhibits a generally elliptical morphology, presenting a smooth light distribution that transitions from a bright, concentrated central region to a fainter, diffuse outer envelope. The core displays a yellowish-white hue, suggestive of an older stellar population. Proceeding outward, the galaxy shows a subtle shift in color, transitioning to a bluish tint in the outer disk, potentially indicative of younger, hotter stars. The shape appears somewhat elongated, but lacks any clear spiral arm structure or signs of significant tidal disturbances. The surface brightness gradually decreases from the center to the periphery. There is a minor suggestion of an extension of the halo on one side, perhaps a small tidal feature, but overall the galaxy appears relatively undisturbed.
