The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The color appears yellowish-white at its core, subtly shifting towards a reddish hue in the outer regions of the disk. There is no apparent spiral arm structure or significant dust lane presence observable in the image, supporting a smooth, spheroidal classification. The galaxy appears relatively isolated, without any readily visible signs of tidal interactions or ongoing mergers with other galaxies. The overall roundedness of the light distribution indicates a morphology that is closer to circular than elliptical, with minimal elongation visible. The object's light distribution suggests a population dominated by older stars. 
