The galaxy presents as a relatively compact object with a smooth, somewhat elliptical morphology. The core region displays a bright, bluish-white hue, suggestive of ongoing star formation or the presence of an active galactic nucleus. This central luminosity is surrounded by a more diffuse, reddish halo. The overall color gradient, transitioning from blue-white at the core to red at the periphery, hints at differential stellar populations and age distribution, with younger, hotter stars concentrated centrally and older, cooler stars dominating the outer regions. There may be some minor disturbances in the galaxy’s morphology, but it is mostly smooth and undisturbed.
