The galaxy exhibits a distorted, disk-like morphology, with evidence suggesting possible tidal interactions or recent merger activity. The central bulge appears bright and somewhat elongated, displaying a concentrated luminosity. A faint, asymmetric halo surrounds the main body, hinting at disrupted stellar populations or ongoing accretion. The disk structure exhibits irregularities and asymmetries; there is a possible sign of a ring-like feature. The colour gradients across the galaxy suggest variations in stellar populations and dust content, with bluer regions potentially indicating areas of active star formation and redder regions associated with older stellar populations or significant dust obscuration. Faint streams or tails extending from the main galaxy are not obvious, but could still be present. It is hard to tell much else due to the limited resolution of the image.
