The galaxy presents a somewhat elongated, cigar-shaped morphology. The central region exhibits a high degree of smoothness and concentration of light. A subtle disk-like structure is discernible, extending outwards from the bright core. The galaxy appears relatively undisturbed, showing no strong signs of a major ongoing merger, although there are hints of minor disturbances in the outer regions. The color profile suggests the presence of both older stellar populations in the central region and relatively younger stellar populations in the outer disk. Overall, this galaxy exhibits characteristics consistent with a transitioning morphology between a pure elliptical and a spiral galaxy.
