The galaxy exhibits a predominantly smooth morphology, lacking prominent spiral arm structures. Its overall shape is elliptical, appearing somewhat elongated or cigar-shaped rather than perfectly circular. The central bulge is noticeable, presenting a concentrated region of light with a yellowish hue. The outer regions of the galaxy gradually fade, showing a diffuse greenish halo suggesting ongoing, but not prolific, star formation. There is no apparent evidence of strong tidal interactions or major mergers, though a slight asymmetry could indicate minor disturbances. Color gradients suggest that the stellar populations are older and redder towards the center, becoming progressively younger with bluer colors in the outskirts.
