The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its overall shape is elliptical, with a noticeable elongation along one axis, transitioning from a bright, nearly homogenous core to a fainter, less defined halo. The color profile suggests an older stellar population, dominated by yellow and red wavelengths. There is little evidence of spiral arm structure or significant dust lanes. Minor asymmetries in the outer regions suggest possible past interactions or minor disturbances, but the dominant impression is one of a relaxed, evolved system. The spatial extent, while moderate, indicates a substantial galaxy.
