This galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution with a slight elongation. There is no apparent spiral structure or dust lanes. The central region displays a yellowish-white color, which likely indicates an older stellar population dominated by evolved stars. Moving outwards from the center, the color gradually shifts to a bluer hue, hinting at the presence of a younger, albeit still relatively quiescent, population. Faint hints of disturbances suggest a possibility of a minor interaction or merger history. The overall morphology and color suggest a relatively passive galaxy with a low rate of star formation.
