The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. There is a slight elongation to the galaxy's shape, but it is mostly round. The lack of distinct spiral arms or dust lanes indicates that this is likely an elliptical galaxy. Faint reddish regions are scattered throughout the galaxy, hinting at the presence of nebulae or regions of ongoing, though relatively subdued, star formation. There are no signs of any major mergers occurring in the image. There may be some minor interactions happening, but any interaction is small relative to the whole.
