The galaxy presents a generally smooth, elliptical morphology. It appears nearly circular on the plane of the sky, exhibiting only a slight elongation. A central bulge region is visible, displaying a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy exhibit a bluer tint, hinting at more recent or ongoing star formation within a disk-like structure. There is a faint indication of what could be a minor tidal disturbance or some other gravitational interaction. Overall, the galaxy appears relatively undisturbed with no prominent merging features.
