The galaxy presents as a moderately bright, elongated structure, likely a disk galaxy viewed at a significant inclination. Its overall color appears slightly blue, suggestive of ongoing star formation, particularly within the disk.

The central region exhibits a somewhat brighter and redder hue than the disk, indicating the presence of an older stellar population, potentially a bulge. The light distribution within the disk appears relatively smooth, with no obvious, large-scale spiral arm structures discernible.

The galaxy's morphology is generally regular. There is no readily apparent evidence of significant tidal disturbances, such as extended plumes or irregular shapes, which would suggest recent major merger activity, although some minor disturbances cannot be ruled out. The galaxy exhibits a moderate degree of elongation, appearing roughly cigar-shaped, indicating it is likely a spiral galaxy viewed from an angle.
