The galaxy presents as a relatively smooth, elliptical-like structure. Its light profile appears centrally concentrated, with a gradual decrease in intensity from the core to the outer regions. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population. The outer regions appear fainter, and have a slight bluish tint, which could suggest the presence of a younger, bluer stellar population. There is no apparent spiral arm structure or dust lane obscuration visible in this image, and the galaxy appears to be in relative isolation, without signs of a major ongoing merger. Based on the slight, irregular shape of the galaxy and the faint, disturbed light on its outskirts, it could be undergoing a minor interaction, however this is difficult to confirm with the information in the image.
