The galaxy appears to be a spiral galaxy, viewed at an oblique angle. Distinct spiral arms are present, exhibiting a flocculent structure. The arms display variations in color and luminosity, suggesting active star formation regions interspersed with older stellar populations and dust lanes.

The bulge component is moderately sized, appearing less luminous than the disk. The overall color of the bulge leans towards the redder end of the spectrum. The disk appears to be the dominant feature of the galaxy. The blue color throughout the disk suggests ongoing star formation. 

There is no obvious evidence of a strong central bar structure. No major merging events or significant tidal disturbances are apparent, although some minor irregularities in the outer disk may indicate past or ongoing interactions.
