The galaxy presents a generally smooth and elliptical morphology, although some disturbed features are visible. The dominant central region exhibits a high degree of symmetry, suggesting a spheroidal component. There is elongation or a slight tidal tail. One side of the galaxy shows evidence of active star formation regions, indicated by a bluer hue, contrasting with the yellower color in the core, which implies an older stellar population. The overall structure suggests a system in the process of merging or experiencing gravitational interaction, as the symmetry of the central bulge is somewhat perturbed. There appears to be a secondary component that is being merged.
