The galaxy appears to be an elliptical galaxy. Its morphology is largely smooth and round, exhibiting a highly concentrated central bulge that fades into a diffuse halo. There is little indication of distinct spiral arms or dust lanes. The galaxy's color gradient suggests that the core is composed of older stars, while the outer regions contain a mix of older and some younger stellar populations. No significant morphological disturbances, such as tidal tails or close companion galaxies, are clearly visible. This indicates the absence of recent major mergers.
