The galaxy presents as a relatively smooth, centrally concentrated elliptical galaxy, with a generally round shape. The light distribution appears fairly uniform, lacking any distinct spiral arm structures or prominent dust lanes. There is a slight color gradient, transitioning from a bluer hue in the center to a redder hue in the outer regions. This suggests a potentially older stellar population dominating the outer parts of the galaxy, with a possibly younger, star-forming population closer to the galactic nucleus. No signs of active galactic nuclei or ongoing major mergers are readily apparent in the image. There may be a slight indication of minor disturbances; however, the image resolution limits a definitive determination.
