The galaxy appears as a centrally concentrated system with a smooth, round morphology, exhibiting a yellow-orange hue suggesting a stellar population dominated by older stars. There is a slight gradient in color, with the central region appearing a more intense yellow. No spiral arm structures or dust lanes are discernible. There is no evidence of any major ongoing merger events or significant tidal disturbances. The overall appearance indicates a galaxy undergoing a relatively quiescent phase of evolution, likely with a low star formation rate.
