The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a concentrated central bulge that fades outwards into a more diffuse halo. There's a slight elongation, deviating from perfect circularity. The galaxy appears to have a relatively passive stellar population, with indications of low star formation activity and a redder color profile. No distinct spiral arms or prominent dust lanes are visible. The general shape is consistent with it being an early-type galaxy which is not actively merging with any other galaxies. 
