The galaxy presents as a somewhat flattened, disk-like structure with a relatively smooth appearance. The central region exhibits a bright, concentrated core emitting primarily in bluer wavelengths, indicative of potentially younger, hotter stellar populations or active galactic nucleus activity. Surrounding the core, there is a less concentrated, broader disk extending outwards, gradually fading into the background. The disk shows subtle variations in color, suggesting some degree of resolved structure. The overall morphology appears undisturbed, lacking prominent spiral arms or significant tidal features suggesting recent major merger activity, although there may be minor disturbances, particularly near the outer edges of the disk. Overall, it appears to be a relatively normal disk galaxy at an unknown inclination.
