The galaxy presents an overall smooth morphology with no apparent spiral arm structure. It exhibits a pronounced central bulge that appears to be significantly brighter and more concentrated than the surrounding disc. The galaxy's shape is elongated, suggesting an elliptical or lenticular classification. The color gradient transitions from a yellowish-white hue at the core to a bluer tint in the outer regions, hinting at possible ongoing star formation in the disc. No signs of major mergers or tidal disturbances are visible. The galaxy may be undergoing minor disturbances, although not clearly apparent.
