The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a roughly elliptical morphology, appearing mostly round but with a slight deviation from perfect circularity. Color gradients are discernible across the galactic structure, with the core region exhibiting a more yellow-orange hue. A small blue area near the edge may indicate regions of star formation. There is no obvious evidence of a strong spiral arm structure or a prominent bar. The overall structure suggests a relatively evolved system. Although there is no clear evidence of major ongoing mergers, some minor disturbances in the outer regions may hint at past interactions or accretion events.
