The galaxy presents a largely smooth, elliptical morphology. It displays a prominent central bulge region that appears relatively bright with a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a bluer color, indicating the presence of younger, hotter stars, albeit less concentrated than in the central bulge. There are some minor indications of a disk-like structure, or at least a flattened distribution of the bluer stellar component, but it is not highly pronounced. There is also a subtle hint of tidal disturbance, but it does not appear to be in the process of actively merging.
