The galaxy presents as a centrally concentrated, smooth object. Its morphology appears to be largely spheroidal, exhibiting a high degree of symmetry without prominent spiral arms or a distinct disk structure. The light is yellowish-white, suggesting a stellar population dominated by older, less massive stars. There are no discernible dust lanes or regions of intense star formation visible in the image. It seems to be a well-formed galaxy with low star formation activity and possibly a relatively high mass. While the galaxy appears largely undisturbed, there is a slight asymmetry in its outer isophotes, which may indicate minor tidal interactions or past merger events, even though it appears mostly undisturbed. The galaxy's light profile decreases gradually from the center outwards, blending smoothly with the background sky.
