The galaxy presents a generally smooth morphology. The central region exhibits a high degree of luminosity, fading gradually towards the outer edges. The overall shape appears elongated, with a discernible cigar-like structure. There is no obvious evidence of spiral arms or a prominent disk. The galaxy shows a dominant smooth component with hints of some disruptions. It exhibits no signs of a recent major merger, although minor disturbances cannot be ruled out. The blue and green colors are indicative of star formation. It has an estimated diameter of about 4.5 kpc. The absolute magnitude suggests a moderately luminous galaxy. It exhibits moderate mass and relatively low star formation rate.
