The galaxy presents as a luminous, disk-shaped structure, elongated along a primary axis. The central region exhibits a bright, concentrated luminosity suggesting a prominent galactic bulge. Moving outward from the core, the brightness gradually diminishes into a more diffuse halo. The overall color appears bluish-white, indicative of a population of younger, hotter stars, although the precise color distribution varies throughout the galaxy. There is evidence of some structural features within the disk, possibly spiral arm segments or dust lanes, but the image resolution limits detailed assessment. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances, though minor irregularities may be present in its outer regions. The shape is neither perfectly round nor highly elongated, occupying an intermediate classification.
