The galaxy presents a generally smooth and rounded morphology. The light profile indicates a centrally concentrated structure, likely a spheroidal component. The color suggests a relatively evolved stellar population, with a dominant yellow hue. There is no obvious evidence of spiral arms or a distinct disk component. The galaxy appears to be relatively undisturbed, with no major signs of tidal interactions or mergers. There may be a slight asymmetry in the outer regions, but this is not pronounced. The galaxy's size appears moderate, and the luminosity suggests a relatively massive system. The lack of blue coloration indicates a low star-formation rate within the galaxy at the time the light was emitted.
