The galaxy presents as an elliptical morphology. It displays a centrally concentrated bulge that appears approximately spherical and smooth, with an orange-red hue suggesting an older stellar population. Extending outward from the central bulge, there is a diffuse, disk-like structure exhibiting a pale blue color, indicative of some younger star formation. The disk component is relatively faint and not sharply defined. There are no distinct spiral arms or prominent dust lanes visible. Overall the galaxy has a soft, blurry apperance due to its distance. There seems to be some minor disturbances.