The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light profile exhibits a smooth, gradual decline in brightness from the center outwards, suggesting a lack of prominent spiral arms or distinct features. The central region shows a concentrated, yellowish hue, indicative of a higher density of older stellar populations and potentially a supermassive black hole. The outer regions fade into a more diffuse, indistinct halo. The overall color gradient suggests a red sequence galaxy, potentially an elliptical or lenticular type, with little ongoing star formation. There may be minor irregularities in the outer regions.
