The galaxy presents as a single, concentrated luminous object with a generally elliptical morphology. The core region exhibits a high degree of brightness with a yellow-orange hue, suggesting an older stellar population. Moving outwards from the central region, the light intensity decreases gradually, transitioning to a broader halo. The outer region exhibits a bluer tint, hinting at younger stars. The overall structure appears relatively smooth, indicating an absence of significant spiral arms or substantial irregularities. There may be some minor disturbances in the outer halo, but no evidence of a major ongoing merger. The galaxy's structure suggests it is either an elliptical galaxy or a spiral galaxy with a very prominent bulge viewed from a nearly head-on orientation. 
