The galaxy presents as a luminous, concentrated central region exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The overall form appears to be spheroidal, with a high degree of radial symmetry, leading to a classification of elliptical. There is evidence of some sort of disturbance, as the galaxy has a distorted shape or irregular features. The galaxy is relatively smooth in its appearance. There is also a smaller object with an orange color. Its relationship with the central galaxy will need to be determined, as it could be an independent galaxy undergoing a merger.
