The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a flattened, disk-like structure with a concentrated central bulge. The light distribution suggests an older stellar population, which is a fairly common feature in such galaxies. There's no distinct sign of spiral arms or active star formation in this image. The galaxy also displays a slight color gradient, becoming more red in the central region and becoming more green towards the outer regions. This implies variations in the stellar population and composition across the galaxy. There's no clear evidence of any major mergers or tidal disturbances, implying that this galaxy has been relatively undisturbed for some time. The shape, while mostly round, does present with a slight elongation, suggesting it is leaning slightly towards being cigar shaped. 
