The galaxy presents a somewhat elliptical morphology. The central region exhibits a high surface brightness, appearing smooth and concentrated with a yellow-white hue. This suggests a dominant population of older stars within the galactic bulge. Moving outwards from the center, the light gradually decreases in intensity. There are hints of a disk structure, indicated by a slightly flattened appearance with patches of blue light that may suggest regions of active star formation. Some faint, disturbed features are visible in the outer regions of the galaxy, possibly due to a minor gravitational interaction. Overall, the galaxy exhibits characteristics of a transitional morphology, appearing neither purely elliptical nor perfectly spiral.
