The galaxy presents a slightly elongated, diffuse morphology with a prominent central bulge. The bulge exhibits a relatively smooth appearance, displaying a concentrated light profile. The outer regions of the galaxy show evidence of a disk-like structure, though it is not sharply defined. Hints of spiral arm features are visible, appearing somewhat flocculent and patchy. The overall color appears to be bluish, suggesting the presence of younger stellar populations and active star formation, though at a moderate rate. There are indications of minor disturbances or interactions, potentially in the form of tidal features or asymmetric structures, particularly in the extended disk. The galaxy does not appear to be undergoing a major merger event, but signs of minor gravitational interactions may be present.
