The galaxy presents a largely smooth and somewhat rounded morphology. It is characterized by a central, luminous bulge that appears reddish in color, suggesting an older stellar population. The bulge gradually transitions into a fainter, more diffuse halo with a bluer hue, indicating the presence of younger stars. There is no clear evidence of spiral arms or a distinct disk structure. Faint irregularities may suggest a minor disturbance or interaction, but the galaxy predominantly appears relaxed and well-formed. The overall color gradient from red at the core to blue in the outer regions is consistent with a galaxy that has undergone significant star formation in the past, with star formation now occurring primarily in the outer regions.
