The galaxy presents as a spiral type, observed at a significant inclination relative to our line of sight. A central bulge is evident, appearing moderately sized and luminous, transitioning smoothly into the surrounding disk. The spiral arms are well-defined, exhibiting a winding pattern of medium tightness, with the majority displaying two prominent arms. These arms are traced by regions of blue coloration, suggestive of active star formation. There is no obvious bar structure. Evident disk features and spiral arm presence suggest the galaxy is not classified as smooth. There is no evidence of a major ongoing merger, and no prominent tidal features or significant morphological disturbance are visible.
