The galaxy presents as a somewhat elliptical, centrally concentrated object. Its core appears bright and yellowish-white, suggesting a population of older stars. The surrounding area shows a subtle, greenish hue, potentially indicating a degree of ongoing star formation or a younger stellar population mixed with dust. The overall structure seems relatively smooth, lacking prominent spiral arms or significant dust lanes visible in this image. There is a suggestion of minor disturbance in the morphology, which could indicate a recent interaction or merger event. The galaxy appears to be relatively massive, with moderate star formation activity based on the color profile.
