The galaxy displays an elongated, cigar-shaped morphology. A slight disk-like component can be perceived, but the overall appearance suggests it is not a well-defined spiral or elliptical galaxy. There is evidence of internal structure with smooth light distribution. The color gradient indicates a mixture of stellar populations, bluer regions possibly hinting at younger stars and star formation and redder regions indicating a population of older, more evolved stars. There is no clear indication of a major merger event, though minor disturbances cannot be ruled out. The galaxy is likely a medium-mass object, potentially with an intermediate rate of star formation.
