The galaxy presents as a barred spiral type. The central bulge exhibits a moderately concentrated, but not dominant, light profile. Spiral arms are discernible but not sharply defined, appearing somewhat flocculent in structure. These arms display a patchy distribution of star formation, evidenced by the presence of bluer regions indicative of younger stellar populations. The disk appears somewhat disturbed, possibly due to tidal interactions or an ongoing merger event. A substantial portion of the galaxy appears affected by some type of disturbance, possibly from a minor or major merger that is ongoing. The bar structure is of moderate strength. The overall color suggests ongoing, though not extremely vigorous, star formation activity.
