The galaxy presents as an elliptical or lenticular morphology with a smooth, concentrated light profile. The central bulge exhibits a strong, yellowish-white luminosity, suggesting an older stellar population and lower star formation rate. The outer regions of the galaxy display a gradual decrease in surface brightness, fading into the background sky. There is some visual evidence of a subtle disk component, hinted by a slight flattening of the galaxy's overall shape. No distinct spiral arms or prominent dust lanes are observed. The galaxy appears relatively undisturbed, lacking any significant signs of ongoing mergers or tidal interactions. Overall, the galaxy presents a mature and well-evolved appearance.
