This galaxy presents a lenticular morphology, displaying a prominent central bulge and a flattened disk component. The bulge region appears luminous and featureless, indicating a high concentration of older stellar populations. The disk exhibits subtle color variations, with hints of bluer regions suggestive of ongoing star formation, especially towards the outer edges of the galaxy. The disk is tilted with respect to our line of sight. The galaxy does not show any signs of major mergers or tidal disturbances, and the smooth appearance suggests it has settled into a relatively stable state. Overall, the galaxy is a well-defined structure, with a clear distinction between the bulge and disk components.
