The galaxy presents a generally smooth morphology, exhibiting a somewhat elongated or cigar-shaped appearance. A bright, concentrated central bulge dominates the galaxy's structure, exhibiting a yellowish hue, which suggests an older stellar population. The bulge gradually fades into a less defined disk. The outer regions display a bluer color profile, possibly indicating regions of more recent star formation. There is no discernible spiral arm structure or any obvious signs of major disturbances or ongoing mergers. The galaxy appears relatively isolated with a high degree of symmetry, and generally appears to be a relatively undisturbed system. 
