This galaxy appears to be an elliptical or lenticular galaxy due to its relatively smooth and featureless structure. The light distribution seems centrally concentrated with a gradual decrease in brightness towards the outer regions. There is a slight elongation evident, although the galaxy presents a generally rounded form. No spiral arms or significant dust lanes are discernible in this image. The galaxy exhibits a bluish hue, possibly indicative of a moderate population of younger stars or ongoing star formation, though the smoothness suggests that star formation activity might be declining or has ceased. A minor disturbance could be present, but it is not conclusive.
