The galaxy presents as a spiral type, with a distinct disk structure. The disk exhibits a relatively high degree of inclination, appearing somewhat edge-on from our viewing angle. Faint, yet discernable spiral arms are visible within the disk, contributing to an overall flocculent appearance. The central bulge is prominent and luminous, showing a yellowish hue, suggesting an older stellar population. Fainter blue regions are observable within the arms, possibly indicating areas of ongoing star formation. No significant signs of a bar structure are apparent in the central region. The overall morphology does not indicate a major ongoing merger event, though minor disturbances can't be ruled out at this resolution. The galaxy appears moderately massive with a rate of star formation that is somewhat suppressed for its mass.
