This galaxy presents as a roughly elliptical structure, exhibiting a notable central bulge that appears bright and concentrated. The color profile suggests a population of older stars, with a yellowish-white hue dominating the central region. Fainter, bluer regions can be distinguished at the outer edges, possibly indicating areas of recent or ongoing star formation, though these features are not sharply defined. There is a subtle disk-like component, evidenced by a slight elongation, though the galaxy does not appear to be a well-defined spiral. The overall morphology hints at an intermediate stage of galaxy evolution, where star formation may be slowing. No significant signs of major disturbances or mergers are immediately apparent in this image. The galaxy's relatively smooth appearance further supports the possibility of it being a post-starburst or quiescent system.
