The galaxy presents a somewhat elliptical morphology. A bright, relatively amorphous central bulge is visually prominent, exhibiting a high degree of luminosity. The galaxy is moderately resolved. Surrounding the central bulge, we observe what appears to be a disk component, extending further outward. The outer regions of this disk show some signs of minor disturbances or irregularities in shape. Overall, the galaxy appears to have some features present, but is mostly characterized by a smooth appearance. There is some possibility of this galaxy having undergone a minor merging event, as indicated by the asymmetry in the outskirts of the disk. The overall color profile suggests active star formation, with indications of younger, bluer stars.
