The galaxy presents as a smooth, elongated structure, suggestive of an elliptical morphology. There is a noticeable color gradient, shifting from a central yellowish hue to a greenish tint along the outer edges. This color differentiation may indicate varying stellar populations or dust distribution. The overall smooth appearance indicates a lack of significant active star formation. There is no strong indication of a merging event or any major disturbance to the galaxy's structure. The galaxy exhibits a moderate redshift, suggestive of a substantial distance.
