The galaxy exhibits a disk-like morphology, appearing highly inclined relative to our line of sight. The central bulge region displays a yellowish-white hue, suggestive of an older stellar population with a lower rate of star formation. Fainter bluish regions are observed in the outer disk, indicative of younger, hotter stars and ongoing star formation. The galaxy shows some slight asymmetry or minor disturbances in its spiral structure. Overall, the galaxy appears to be an intermediate mass system with moderate star formation activity.
