The galaxy appears as a singular, rounded structure, generally smooth in overall texture. The central region exhibits a brighter, concentrated luminosity, potentially indicating a dense stellar population or active galactic nucleus. A diffuse, lower-intensity halo surrounds the core, fading gradually into the background. Color gradients are subtle but present, with a slight shift towards bluer hues in the outer regions, possibly suggestive of younger stellar populations engaged in active star formation. No distinct spiral arms or bar structures are visually discernible. Minor asymmetries or disturbances in the outer regions may be indicative of past or ongoing interactions with smaller companions, but are difficult to confirm based on this observation alone. The overall morphology is consistent with an elliptical or early-type spiral galaxy.
