The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white hue, indicative of an older stellar population dominating the central regions. A slight elongation is observed, suggesting a deviation from a perfectly spherical shape. The outer regions show a gradual decrease in surface brightness, fading into the background sky. There is evidence of faint, reddish coloration in a small section of the galaxy, which might suggest regions of ongoing star formation. There are no obvious signs of a prominent disk structure, spiral arms, or major tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
