The galaxy presents a morphology consistent with a spiral type, viewed at an oblique angle relative to our line of sight. Distinct spiral arm structures are visible, albeit somewhat blurred, suggesting a relatively high degree of symmetry and order. The arms exhibit a flocculent structure.

A prominent central bulge is observed, displaying a smooth, concentrated luminosity profile. The bulge appears substantial, contributing significantly to the overall luminosity of the galaxy. The light from the bulge appears somewhat yellower than the light from the disk. A possible bar structure may be present extending throughout the inner disk, however it is hard to distinguish.

The disk component displays a bluer color, indicative of ongoing star formation. The galaxy appears to be relatively isolated, showing no obvious signs of interaction or merging activity.
