The galaxy presents as a centrally concentrated object, appearing largely smooth with a hint of elongation. The light distribution suggests a predominantly elliptical morphology, lacking any obvious spiral arm structures or bar features. The core exhibits a high surface brightness, transitioning to a more diffuse outer halo. There is a slight color gradient visible, with a central region that appears more reddish, possibly indicating an older stellar population, surrounded by a bluer hue, which could denote more recent star formation activity. Overall, the galaxy seems to be relatively undisturbed, with no obvious signs of ongoing mergers or tidal interactions.
