The galaxy presents a generally smooth and elliptical morphology, with a concentrated central bulge. The bulge exhibits a yellowish hue, indicative of an older stellar population. The outer regions of the galaxy appear more diffuse, transitioning to a slightly redder color. There is a subtle hint of disk-like structure, with a very slight flattening, but no obvious spiral arms or strong features are visible. The galaxy appears relatively undisturbed with no indication of a major ongoing merger.
