The galaxy presents a flattened, elongated morphology, suggestive of a spiral or lenticular type, seen at a significant angle relative to our line of sight. The central region exhibits a bright, concentrated luminosity, indicating a substantial stellar population, possibly an older bulge. Moving outwards from the core, the light fades gradually, displaying a smooth profile without prominent spiral arm structures, or particularly bright star-forming regions. The overall color of the galaxy is relatively uniform, with a tendency towards redder hues in the central bulge and slightly bluer hues toward the edges of the disk, hinting at a lower rate of current star formation, with hints of underlying dust obscuration. There might be a minor disturbance in the overall symmetry of the galactic shape.
