The galaxy presents a largely smooth morphology, lacking prominent spiral arms or a distinct disk structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards. The galaxy exhibits a generally elliptical shape, appearing nearly circular with only a slight deviation from perfect roundness. There is no strong indication of ongoing major mergers or significant tidal disturbances, although subtle features suggest the possibility of minor interactions or past accretion events. The galaxy appears to be a fairly mature system, with a relatively low rate of star formation and correspondingly redder colors indicative of an older stellar population. Overall, the galaxy is best described as a quiescent elliptical galaxy with a relatively smooth and featureless appearance.
