The galaxy presents a generally smooth and rounded morphology, suggesting an elliptical or lenticular classification. It exhibits a central concentration of light, potentially indicative of a bulge. There is a slight elongation observed, but it is not strongly barred or spiral in nature. The color profile appears bluer in the central regions, possibly indicating more recent star formation activity compared to the outer regions. No major disturbances or signs of on-going mergers are immediately apparent, although a minor asymmetry exists in the upper left. The galaxy appears relatively isolated, with no other large galaxies in close proximity.