The galaxy presents a dominant, elongated, and somewhat smooth morphology. Its form suggests a spheroid with an axis ratio significantly deviated from unity, lending it a cigar-like appearance. A possible disk-like structure may exist given the color variations. The light profile appears relatively smooth, with a centralized condensation, however a slight asymmetry might indicate minor disturbances, possibly due to a weak tidal interaction or past merger event. Integrated light indicates moderately low star formation activity. The overall color is slightly bluer than typical quiescent galaxies at this distance.
