The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. Its light profile indicates a high degree of radial symmetry, deviating only subtly from a perfect circle. There are no strong indications of spiral arm structure, bar features, or prominent dust lanes within the visible portion of the galaxy. The overall color suggests a relatively older stellar population, with a noticeable absence of intensely blue regions indicative of vigorous, ongoing star formation. Subtle color gradients are present, potentially suggesting radial variations in stellar population or metallicity. There is possible minor disturbance present.
