The galaxy presents a largely smooth, elliptical morphology, with a high degree of central concentration. The light distribution appears relatively uniform, with a gradual decrease in intensity from the core to the outer regions. The galaxy exhibits a subtle elongation but is largely round, with a slight cigar shape, hinting at a possible departure from perfect sphericity. There is a hint of a reddish hue, particularly in the central region, which may be due to an older stellar population. There is no obvious disk component or spiral arm structure. Based on its morphology, this galaxy is likely an early-type system. A possible minor disturbance appears to exist in the structure of the galaxy, possibly due to some kind of disruption.
