The galaxy exhibits a largely smooth morphology, suggestive of an elliptical or lenticular type. The light distribution appears centrally concentrated with a diffuse, extended halo. The overall color is somewhat intermediate, showing a mixture of redder and bluer hues, concentrated toward the core. There is little evidence of distinct spiral arms or a prominent disk structure. Given the smoothness and color profile, this galaxy may have a relatively low star formation rate. The concentration of light towards the center may indicate a prominent galactic bulge or a central supermassive black hole. There appears to be no ongoing major merger event, though there may be minor disturbances within the galaxy. The galaxy appears mostly in between round and elliptical. No cigar shaped is observed.
