The galaxy presents as a relatively smooth, centrally concentrated structure, though not perfectly spherical. There appears to be a slight elongation or asymmetry to its overall shape. Its color profile suggests an older stellar population, with a dominant yellowish-orange hue in the central regions, indicating a lack of significant ongoing star formation. Faint bluish extensions can be observed on the edges of the galaxy, which may indicate the presence of younger, bluer stars, or perhaps tidal debris resulting from minor gravitational interactions. There is no strong evidence of a prominent disk or spiral structure. No signs of significant ongoing merging activity are apparent. The galaxy appears to be a fairly massive system, based on its overall brightness and apparent size.
