The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. Its shape is elongated, presenting a cigar-shaped profile. The galaxy demonstrates a concentration of light towards its center, with a gradual decrease in brightness towards its outer edges. There is no evidence of spiral arms or a distinct disk structure. The central region displays a slightly yellowish hue, possibly indicating an older stellar population, while the outer regions exhibit a bluer tint, suggesting the presence of younger stars, though their proportion appears small. The galaxy shows no signs of major mergers or significant disturbances in its structure.
