The galaxy presents as a spiral type, exhibiting a notable disk structure with a moderate bulge. The disk appears to be inclined relative to our line of sight. Traces of spiral arms can be observed emanating from the central bulge, although they are not sharply defined, appearing somewhat flocculent. The bulge itself shows a yellowish hue, suggestive of an older stellar population, while the disk reveals a bluer tone, indicating ongoing star formation. There may be a weak bar structure bisecting the central bulge. No significant signs of major disturbances are apparent.
