The galaxy presents as a relatively smooth, elongated structure, likely an elliptical galaxy viewed at an angle. The central region exhibits a concentration of light, suggesting a dense stellar population or possibly an active galactic nucleus, though without spectroscopic data, this remains speculative. There is a color gradient within the galaxy, with the central bulge appearing more yellow, possibly indicating an older stellar population, and the outer regions showing hints of blue, potentially signifying younger stars. No distinct spiral arms or dust lanes are discernible in the image, further supporting the classification as an elliptical or lenticular galaxy. There is no indication of a major ongoing merger, though there may be some minor disturbances in the outer regions.
