The galaxy appears as a relatively smooth, elliptical-like structure, with a bright, concentrated central bulge. There is a distinct color gradient, transitioning from a yellowish-white core to a bluer halo. The central core is approximately 5 kpc in radius. There is little evidence of spiral arms or a disk structure, however the slight blue tint toward the outer edges suggests the presence of some ongoing star formation. Overall, the galaxy exhibits a fairly undisturbed morphology, showing no signs of a major merger event. There is some evidence for minor tidal disturbance that might be causing the on going star formation.
