The galaxy appears to be a relatively smooth, centrally concentrated system. The core exhibits a yellowish hue, potentially indicating an older stellar population. There is a gradual decrease in surface brightness outwards from the center with a moderate ellipticity. Some subtle irregularities are visible in the outer regions of the galaxy, hinting at possible minor disturbances or interactions. The galaxy appears to be neither a pure elliptical nor a spiral, perhaps an intermediate type. It doesn't show significant ongoing star formation and doesn't show any signs of a major merger event, although the minor disturbances could suggest it is interacting with a nearby object. Overall, the galaxy appears to be a relatively quiescent system, likely located at a substantial cosmological distance.
