The galaxy appears as a relatively small, elongated object with a flattened disk-like structure. It exhibits a predominantly blue hue, suggesting a younger stellar population and ongoing star formation. The light intensity distribution appears relatively smooth, with no distinct spiral arm structures readily visible. The central region presents a slightly brighter, more concentrated area, possibly indicating the presence of a bulge. The overall shape is suggestive of a disk galaxy viewed at a considerable inclination angle. Some areas have the suggestion of faint patchiness within the disk, which may suggest areas of ongoing star formation and a non-uniform distribution of interstellar dust. There is a subtle hint of possible tidal disturbances or interactions, but this assessment would require further higher-resolution imaging to confirm.
