The galaxy appears to be an elliptical type, characterized by a smooth, featureless morphology. It exhibits a centrally concentrated luminosity profile, with the light intensity decreasing gradually towards the outer edges. The color gradient suggests an older stellar population, particularly evident in the reddish-orange hue of the core. There is no apparent spiral structure or distinct dust lanes. The galaxy appears relatively round, with only a slight deviation from perfect circularity. There is no obvious evidence of any major ongoing merger activity or significant tidal distortions in the galaxy's shape. Faint blue light is observed in a ring shape around the central bulge, which could suggest the formation of younger stars.
