The galaxy presents as a fairly smooth, round structure with a concentrated central region. There is a distinct lack of discernible spiral arms or other prominent features typically associated with disk galaxies. The light profile appears to decrease gradually from the core outwards. A subtle color gradient is observed, with the central region exhibiting a slightly bluer hue compared to the redder outer regions. No significant morphological disturbances are visible. The galaxy presents a mostly undisturbed, elliptical or lenticular-like appearance, with a dominant smooth component.
