The galaxy exhibits an overall elliptical morphology, appearing as a flattened spheroid. The light distribution is centrally concentrated, with a bright, well-defined core. Moving outwards from the core, the intensity gradually decreases, forming a diffuse halo. Some faint disk-like structure is visible, exhibiting a slight tilt relative to the line of sight. The axial ratio indicates that it is moderately elongated. The color gradients suggest older stellar populations dominate the central region, with bluer colors and signs of possible star formation in the disk. There is no evidence of strong spiral arm features or a prominent bar. It displays no strong signs of ongoing merger activity or tidal disturbances.
