This galaxy exhibits a disk-like structure, although it presents with some irregularities. There is evidence of possible disturbances or interactions, as the morphology deviates from a perfectly smooth or symmetrical form. The galaxy displays a central bulge that appears relatively bright and concentrated. Star formation activity is apparent in the disk, with some regions showing a bluer color indicative of younger stellar populations, though the overall star formation rate seems subdued. The disk itself shows some patchiness, and there might be faint tidal features or asymmetries suggesting a past or ongoing merger event.
