The galaxy presents as a largely smooth, elliptical-type system. Its morphology is dominated by a central bulge exhibiting a radial color gradient, transitioning from a yellowish core to a more reddish outer halo. There's little evidence of significant spiral arm structure or active star formation regions. The galaxy displays a relatively round shape, deviating only slightly from a perfect circle. No major tidal distortions or signs of ongoing major mergers are visually apparent, though subtle asymmetries and minor disturbances cannot be entirely ruled out at this resolution. The galaxy appears to be relatively isolated in its immediate vicinity. Overall, the galaxy's appearance is consistent with that of a massive, evolved system with a diminished star formation rate.
