The galaxy appears to be an elliptical type with a smooth, generally featureless morphology. It exhibits a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. There is a subtle color gradient across the galaxy, with the central regions appearing more yellow-red and the outer regions tending towards green, implying variations in stellar population or dust content. There seems to be a possible minor disturbance in the bottom of the image, with an object appearing to merge. The galaxy is generally isolated and no strong evidence is found of a strong recent merger.
