The galaxy appears to be an elliptical system, exhibiting a smooth, centrally concentrated morphology. There is evidence of an extended halo surrounding the core, which indicates a significant stellar population distributed beyond the main body. The color profile is generally redder, suggesting an older stellar population with lower levels of ongoing star formation. No distinct spiral arms or prominent dust lanes are visible. There are some minor visual disturbances, and it seems possible that it is undergoing a minor merger with another galaxy. The object is quite round, but not perfectly so, having a more oblate shape.
