The galaxy presents a generally smooth morphology, with a significant central bulge region exhibiting a yellowish hue. Surrounding the bulge is a fainter, more diffuse halo or disk-like structure, which appears greenish. This suggests a difference in stellar populations, with the bulge potentially populated by older, redder stars, and the disk containing younger, bluer stars.

The overall shape of the galaxy is approximately round, though there's a slight elongation or flattening visible, hinting it is either transitioning to a disk structure, or is possibly affected by tidal interactions. There is no strong evidence of a major merger event, but there seems to be an indication of a minor disturbance in the smooth structure of the outer regions. The color distribution is mostly uniform, further solidifying the smooth classification. 
