The galaxy presents an elliptical morphology, appearing largely smooth and well-rounded in shape. The core exhibits a bright, concentrated luminosity that gradually decreases towards the outer edges, suggesting a high stellar density within the galactic nucleus. The color gradient transitions from a yellowish-white core to a reddish hue in the outer regions, potentially indicative of an aging stellar population in the galaxy's halo. There is no visible evidence of spiral arms or prominent dust lanes. There are no significant tidal disturbances or merging features discernible, implying the galaxy is relatively undisturbed.
