The galaxy presents as a spiral with a moderate inclination relative to our line of sight. The central bulge appears relatively small and dim, gradually transitioning into the spiral arms. The arms themselves are tightly wound, displaying a flocculent structure with regions of enhanced brightness indicative of active star formation. These regions are bluer in color, suggesting a younger stellar population. Dark dust lanes are subtly visible along the inner edges of the spiral arms, obscuring some of the light from behind. The overall morphology suggests a late-type spiral galaxy, possibly of type Sc or Sd. There appears to be a slight asymmetry in the distribution of light in the outer regions, which might be due to tidal interactions, though no clear companion galaxy is visible in the immediate vicinity. There is no apparent bar feature.
