The galaxy presents a generally smooth morphology, exhibiting characteristics somewhere between elliptical and disk-like. The light distribution appears largely homogeneous without prominent spiral arm structures or significant dust lane obscuration. The central region displays a high concentration of light, indicative of a galactic bulge. The galaxy is not perfectly round, but its light distribution is not extremely elongated either. There are no obvious signs of major merging events. The bluer color at the bottom may imply higher star forming rate in that region, but it is only slightly prominent. Overall, this galaxy seems to be fairly quiescent, with most stars being older.