The galaxy presents as a relatively smooth, elliptical morphology. Its overall shape appears elongated, exhibiting a cigar-like appearance. The central region shows a concentration of light, indicating a prominent galactic bulge. The galaxy is composed primarily of older stellar populations, emitting light in the redder end of the spectrum, with only mild recent star formation present. There is no evidence of significant dust lanes or spiral arm structures. The overall structure suggests a relaxed system that has undergone significant morphological transformation with little evidence of tidal disturbances or recent mergers. The galaxy is an estimated 4 kpc across, with an intermediate mass.
