The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile. The object displays an overall yellowish-white hue, concentrated towards its center, suggesting a relatively older stellar population dominating the core. The outer regions of the galaxy exhibit a more subdued coloration, hinting at either a less dense distribution of stars or the presence of a mixed population with some younger, bluer stars. The galaxy appears elongated, with a moderate degree of ellipticity. There is no visible evidence of spiral arms or strong dust lanes. The overall structure suggests a system that has undergone significant merging activity in its past, leading to the homogenization of its stellar components.
