This galaxy presents a lenticular or early spiral morphology. It is characterized by a prominent, bright, and somewhat elongated central bulge. The bulge exhibits a yellowish-orange hue, indicative of an older stellar population. A flattened disk extends outwards from the bulge, with a noticeable blueish tint in some regions, suggesting the presence of younger, hotter stars and ongoing star formation, albeit at a low rate. No distinct spiral arm structure is readily apparent. The galaxy appears relatively undisturbed, with no obvious signs of recent major merger events. Overall, the galaxy exhibits a smooth, consolidated structure.
