The galaxy presents as an elliptical morphology, elongated with an approximate axis ratio of 0.6. The central region exhibits a bright, concentrated core, suggestive of a bulge component. A gradual decline in surface brightness is observed moving outward from the core, transitioning into a smoother, more diffuse halo. The color profile appears redder towards the central bulge, indicating an older stellar population. Fainter, bluer hues are seen in the outer regions of the galaxy, potentially indicating the presence of younger stars. Overall, the galaxy appears relatively undisturbed, lacking prominent tidal features or distortions. The galaxy shows an inclination that makes it appear slightly elongated from our point of view.
