The galaxy presents as an elliptical morphology, with a high degree of central concentration. The core exhibits a bright, yellowish hue, possibly indicating an older stellar population. Surrounding the core is a less luminous region, showing a subtle blueish tint. The outer regions of the galaxy gradually fade into the background sky. The galaxy appears relatively smooth, with no obvious signs of spiral arms or significant dust lanes. The ellipticity suggests a slightly flattened shape. There does not appear to be any evidence of ongoing major mergers or strong tidal interactions.
