The galaxy presents as a roughly elliptical object, appearing smooth with a concentrated central bulge and a more diffuse halo. It exhibits a predominantly yellowish-orange hue, suggesting an older stellar population with minimal ongoing star formation. There is a slight elongation, deviating from a perfectly circular shape. No distinct spiral arm structures are apparent, indicating it is most likely an elliptical galaxy with little discernible disk component. There are also subtle irregularities to its structure which may indicate there was a previous minor merger event.
