The galaxy presents a smooth, elliptical morphology. There is little evidence of spiral arms or significant disk structures. The galaxy exhibits a roughly round shape, with a slight elongation. The color profile indicates a central bulge that is yellowish, suggesting an older stellar population. Fainter blue hues are detected at the edges, potentially indicating ongoing star formation. Overall, the galaxy appears to be relatively undisturbed, with no clear signs of major mergers or tidal disruptions.
