The galaxy appears to be a relatively smooth and rounded system. A bright, concentrated central bulge is observed, which transitions smoothly to a fainter, extended halo. The overall color gradient suggests a concentration of older stellar populations in the bulge, with bluer colors possibly indicating ongoing star formation in the outer regions, although this is not clearly discernible from the image. There is no obvious spiral structure or prominent dust lanes. There might be a minor disturbance in the symmetry suggesting there may have been a minor interaction, but overall the galaxy seems fairly undisturbed.
