The galaxy presents as a generally smooth object with a slight ellipticity, appearing more "in-between" than perfectly round or cigar-shaped. A central bulge dominates the galaxy's luminosity profile, exhibiting a yellowish-white hue. The outer regions of the galaxy are more diffuse, with a gradual decrease in brightness away from the center. There is no evidence of strong spiral arm structures or significant dust lanes. There is only a slight possibility of a minor disturbance in the disk. Based on these observations, the galaxy is likely an early-type spiral or lenticular galaxy with a relatively high degree of central concentration and minimal ongoing star formation.
