The galaxy appears as a centrally concentrated object with a largely smooth morphology. It exhibits a generally elliptical shape, appearing moderately rounded rather than elongated. The light distribution suggests a dominant spheroidal component. There is faint hint of possible disk like structure. The galaxy's color index indicates a relatively mature stellar population. No prominent spiral arms or significant dust lanes are discernible in this image. There is no obvious evidence of recent or ongoing major mergers or tidal disturbances. The smooth appearance suggests that the galaxy is not undergoing intense star formation activity and has likely undergone some amount of quenching. 
