The galaxy appears to be a spiral galaxy observed at an inclination, presenting an elongated, cigar-shaped profile. A bulge is visible, transitioning smoothly into a disk structure. The light from the galaxy indicates a mix of stellar populations, showing blue-green hues which are prominent in some regions. The galaxy appears to have a high degree of smoothness within its structure, suggesting it is not undergoing any major merging events. There is some indication of minor disturbance, such as asymmetry. Star formation is likely occurring. The galaxy appears to be a relatively massive system with moderate star formation activity.
