The galaxy presents a flattened, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly spherical and gradually decreasing in intensity towards the outer regions. It has a slight bulge. The orientation of the major axis is apparent, and the galaxy exhibits a smooth texture, with little evidence of distinct spiral arms or significant dust lanes. The galaxy appears to be relatively isolated and the color indices indicate the presence of an aging stellar population with the possibility of on-going star formation.
