The galaxy presents as a relatively compact and centrally concentrated structure. It exhibits a predominantly smooth morphology, lacking prominent spiral arms or a distinct disk-like appearance. The overall shape appears slightly elongated, tending towards an elliptical form rather than a perfect sphere. The color profile suggests a dominant population of older stars, contributing to a yellow-red hue, especially in the central bulge. There's a hint of a bluer, potentially younger stellar population towards the center as well. No signs of active galactic nuclei or recent major mergers are immediately apparent in this image. Faint irregular features imply there might be a low level of on-going star formation within this galaxy.
