The galaxy presents as a distorted, disk-like structure with an overall bluish hue, suggestive of ongoing star formation. One section appears more prominent, exhibiting a more condensed region likely housing a bulge or a concentration of older stars. The morphology suggests a system that has potentially undergone gravitational interactions or minor mergers. The light distribution exhibits some asymmetries, possibly indicating tidal features or disturbances in the galactic disk. There's a slight color gradient noticeable, with bluer regions primarily observed toward the outer regions of the disk, consistent with a spiral-type galaxy undergoing star formation.
