The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with no apparent spiral arm structures or a distinct bulge. The galaxy's color profile suggests a dominant older stellar population, indicated by the reddish-yellow hue. There's a slight hint of asymmetry in the outer regions, which could imply a possible tidal interaction or past merger event. Overall, the galaxy presents a quiescent nature with minimal evidence of ongoing star formation.
