The galaxy presents with a distinct, somewhat elongated morphology. It appears to have a bright, concentrated central bulge region that contributes significantly to the galaxy's overall luminosity. Surrounding the bulge is a discernible, though not sharply defined, disk component.

The disk displays a mottled texture, potentially indicative of active star formation regions or dust lanes. The disk component does not appear entirely uniform; there are subtle variations in color and brightness suggesting underlying structural features.

Overall, the galaxy does not exhibit pronounced spiral arm structure. There is evidence of minor asymmetry or distortion in the galaxy's shape, particularly in the disk, which could be indicative of a past interaction or merger event.
