The galaxy presents a largely smooth morphology, indicative of an elliptical or lenticular type. A bright central bulge dominates the structure, with a gradual decrease in luminosity towards the outer regions. The core exhibits a yellowish-white hue, potentially suggesting an older stellar population with reduced ongoing star formation. The outer regions show a slight hint of blue, which might indicate the presence of some younger, hotter stars, albeit at a lower rate than typically seen in spiral galaxies. The overall shape appears relatively round with no distinct spiral arms or bar-like features. There are no obvious signs of tidal disturbances or interactions with other galaxies, suggesting a gravitationally relaxed and relatively undisturbed system. Based on the color profile, it is likely a massive galaxy.
