The galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology with a high degree of central concentration. The light is concentrated towards the center with a clear radial gradient. The galaxy exhibits a yellow-white hue centrally, fading to a blue-white in the outer regions, suggesting a population of older stars dominating the core, with evidence of possibly some younger stars towards the periphery. There is a noticeable absence of distinct spiral arm structures or dust lanes, supporting its classification as an elliptical galaxy. The overall structure appears relatively undisturbed, with no signs of major mergers or tidal disruptions. There may be some evidence of minor disturbances but more data would be needed to confirm this.
