The galaxy presents as a centrally concentrated, smooth light distribution. The object exhibits a spheroidal morphology with a high degree of central symmetry. There is a color gradient from the center outwards, with the core appearing more yellow/white, indicative of older stellar populations, and the outer regions exhibiting a slightly redder hue. No distinct spiral arm structures or prominent dust lanes are discernible. The overall appearance suggests an elliptical galaxy or a lenticular galaxy seen face-on, with little evidence of ongoing star formation. The galaxy appears relatively undisturbed, with no signs of major mergers or tidal interactions. A slight asymmetry may indicate minor interactions.
