The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, appearing yellowish in color. The outer regions of the galaxy gradually fade into a bluish hue, suggesting the presence of younger stellar populations. The overall morphology hints at a disk-like structure viewed at a significant inclination angle. There is no obvious evidence of a spiral arm structure or bar. The galaxy appears relatively undisturbed, with no major signs of ongoing merging events, although a slight asymmetry on one side suggests a possible minor interaction in its past. The galaxy's light distribution appears smooth, indicating a relatively evolved system with ongoing, yet potentially limited, star formation activity.
