The galaxy presents as a spiral type, inclined significantly relative to our line of sight. Spiral arm structure is discernible, though not sharply defined. The arms appear somewhat flocculent, and the overall structure suggests a barred spiral configuration. The central bulge is moderately sized, exhibiting a yellow-white color suggesting an older stellar population. The disk component appears bluer, indicative of ongoing star formation. There is some asymmetry and irregularity evident, which may be indicative of minor interactions or internal disturbances within the galaxy.
