The galaxy presents as a somewhat disturbed system. There is evidence of a disk-like structure, though it is not clearly defined and appears to be viewed at a slight inclination. A prominent central bulge dominates the galaxy's light profile, appearing with a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions are visible within the disk, implying pockets of ongoing star formation. The overall structure exhibits irregularities, potentially indicating tidal interactions or recent merger events. The disk shows some asymmetry, which may result from gravitational disturbances.
