The galaxy appears to be an elliptical type. It exhibits a smooth, centrally concentrated light profile. The shape is elongated, with a noticeable departure from a perfectly circular morphology. There is a bright, yellowish core that decreases in intensity gradually towards the outer edges of the galaxy. Hints of blue are subtly visible in the extended halo, particularly at its edges, suggesting some presence of younger stellar populations. No obvious dust lanes or spiral arm structures are detected. No strong tidal features or signs of recent major merger activity are visible, though there might be some minor disturbances in the halo.
