The galaxy presents as an elliptical-like system, exhibiting a smooth, diffuse morphology with no discernible spiral arm structure or dust lanes. The light distribution is centrally concentrated, showing a gradual decrease in intensity outwards from the core. The central region appears brighter and possesses a slightly reddish hue, potentially indicating a population of older stars. Moving outward, the color shifts towards a slightly bluer tone, which could be indicative of a younger stellar population forming in the outer regions. Overall, the galaxy appears elongated and relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
