The galaxy appears as a slightly elongated, centrally concentrated object. Its overall color profile suggests the presence of both younger and older stellar populations. The core region exhibits a pronounced redder hue, potentially indicative of an older population of stars or significant dust obscuration. Surrounding the core, a diffuse, greenish-blue halo is visible, implying the presence of younger, hotter stars or ongoing star formation. The galaxy does not exhibit a clear spiral structure or distinct features like prominent arms, suggesting it may be an elliptical or lenticular galaxy. There are slight disturbances in the halo, but nothing to suggest a major merger. Overall, the galaxy seems to be relatively smooth in appearance with intermediate roundness.
