The galaxy appears to be a relatively smooth, centrally concentrated object. The morphology indicates a primarily elliptical or lenticular galaxy. It is predominantly yellowish-orange in color in its central region, indicating an older stellar population. The outer regions have a slightly bluer hue, suggesting the presence of some younger stars or ongoing star formation, though at a very subdued rate. There is no apparent evidence of a distinct disk structure or prominent spiral arms. No signs of significant tidal disturbances, or major mergers are visible, suggesting it has likely experienced a relatively quiescent evolutionary history recently. The overall shape of the galaxy is somewhat elongated but mostly round.
