The galaxy presents as a smooth, elliptical-like structure. Its core exhibits a concentrated luminosity, suggesting a high density of stars. The light emanating from the galaxy displays a noticeably redder hue than the background sky, potentially indicating an older stellar population and/or significant dust obscuration within the galaxy itself. Its overall shape deviates somewhat from a perfect ellipse, displaying hints of distortion. There's also some evidence of an asymmetric distribution of light in the outer regions, although it remains subtle.
