The galaxy presents as a relatively compact object with a discernible central bulge. The overall color profile suggests a population of older stars, although the presence of some bluer regions indicates ongoing, albeit subdued, star formation. The galaxy appears largely elliptical in nature, exhibiting a smooth morphology with minimal evidence of spiral arms or significant dust lanes. There's a slight elongation observable but not in the extreme. The galaxy does not show any strong signs of tidal disturbances or major mergers, though a possible minor interaction cannot be completely ruled out based on its overall asymmetric glow.
