The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents an elliptical, elongated shape. There is no clear evidence of spiral arm structure. The central region is brighter, but there is no distinct, well-defined nucleus. Fainter, diffuse light extends outwards from the central region. There is no obvious dust lane or any pronounced indication of recent major merger activity, though subtle signs of minor disturbances may be present. Color gradients within the galaxy are subtle, with a possible tendency towards redder colors in the central regions.
