The galaxy presents as a centrally condensed object with a flattened, disk-like morphology. The central region appears bright and somewhat amorphous, lacking clear spiral structure. Distinct color gradients are observed, with a central yellowish-red core transitioning to bluer hues in the surrounding regions. There is a slight asymmetry along the horizontal axis, suggesting possible tidal interactions or internal disturbances. There is little evidence of distinct spiral arms, however some subtle features could indicate a weak or disrupted spiral pattern, or a ring structure. The galaxy exhibits a relatively small angular size, likely indicating a significant distance.
