The galaxy presents as a slightly elongated, disk-like structure. The central bulge exhibits a yellowish hue, suggesting a population of older, cooler stars, or significant dust obscuration. Surrounding the bulge is a less defined disk, with faint spiral arm structures visible. These arms display a slightly bluer color, indicative of ongoing star formation. There is a subtle asymmetry in the disk, potentially hinting at a past minor merger or tidal interaction, as indicated by what seems to be a minor disturbance in its form. Overall, the galaxy appears to be a massive system with ongoing star formation, though possibly at a moderate rate.
