The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a predominantly elliptical morphology, appearing more 'in between' round and cigar shaped, than perfectly circular. The color profile indicates a likely evolved stellar population, displaying a yellowish to reddish hue. This suggests a relatively low current rate of star formation. There are no prominent dust lanes or spiral arm structures visible, further supporting the classification as a smooth galaxy. There is no obvious evidence of any major merging activity or tidal disturbances. Overall, the galaxy appears to be a well-formed, undisturbed system.