The galaxy presents a primarily smooth and centrally concentrated morphology. There appears to be a bright, compact nucleus, possibly indicating an active galactic nucleus or a dense stellar population in the core. The main body of the galaxy exhibits a slightly elongated shape, deviating somewhat from perfect sphericity. Faint extensions are possibly observed from the galaxy. Given the apparent smoothness and lack of obvious spiral arms or irregular features, it is likely a galaxy of an elliptical or lenticular type. Minimal to no evidence of ongoing major mergers or significant tidal disturbances is observed. The color indices suggest a stellar population with a lack of extremely young stars.
