The galaxy presents an overall elliptical morphology, exhibiting a smooth light distribution with no obvious spiral arm structures. The central region is bright and concentrated, indicating a significant bulge component. Moving outward, the light gradually fades into a diffuse halo. The galaxy's shape appears moderately elongated, exhibiting a slight cigar shape rather than a perfect circle. There are no signs of major mergers or tidal disturbances. Faint, diffuse features may be indicative of minor interactions. There is evidence of low-level star formation throughout the galaxy.
