The galaxy presents as a relatively smooth, somewhat elliptical structure. A concentrated central bulge exhibits a distinct yellowish-orange hue, suggesting an older stellar population and potentially less ongoing star formation in that region. Surrounding the core is a diffuse, bluish halo or disk. This outer region indicates the presence of younger, bluer stars and potentially active star-forming regions, though they are not clearly resolved in the image. There is a subtle hint of a spiral structure; however, it isn't well-defined and may indicate that the galaxy is a late-stage spiral or transitioning into an elliptical galaxy. There's no obvious evidence of strong tidal disturbances or ongoing major mergers, although there could be minor irregularities in the outer regions suggesting past interactions. The overall color gradient, transitioning from reddish-yellow in the core to bluish in the outer regions, is consistent with a galaxy that has ceased its star forming activity in the core.
