The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The galaxy appears to be highly spheroidal in shape, exhibiting a slight elongation. The central bulge dominates the overall structure. There is a noticeable color gradient, with the core appearing more yellowish-white and the outer regions exhibiting a slightly redder hue. Evidence for spiral arms is absent, reinforcing the classification of this galaxy as elliptical. No signs of major disturbances or ongoing mergers are visibly apparent, though some minor irregularities are present that could indicate minor disturbance. The object appears relatively isolated, with no other galaxies appearing to interact with it within the immediate vicinity.