The galaxy presents a cigar-shaped morphology, appearing highly elongated along its major axis. The light distribution suggests a dominant bulge component with a smooth, diffuse appearance. There is some evidence of a faint disk structure, though it is not sharply defined and appears relatively featureless. The galaxy exhibits a color gradient, with the central bulge appearing more yellow/orange and the outer regions trending towards bluer hues. This could indicate a difference in stellar populations, with older, redder stars concentrated in the bulge and younger, bluer stars in the disk. There is no obvious indication of active star formation or prominent spiral arms. It is possible that the galaxy is undergoing minor interactions, but overall it appears relatively undisturbed. Based on its morphology, it appears to be a galaxy that has undergone significant evolution, likely with a high fraction of older stars.
