The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a hint of disk-like structure, although it is not sharply defined. The galaxy appears somewhat elliptical in shape, with a moderate degree of elongation. The central region exhibits a pronounced yellow-orange hue, suggesting a relatively older stellar population, or a substantial dust component. Fainter, more diffuse light extends outwards from the central region. Evidence of any major disturbances or ongoing mergers is not readily apparent, though subtle asymmetry may indicate a minor interaction in the past. Overall the galaxy appears as a fairly massive system with little current star formation.
