The galaxy presents as a relatively smooth, elongated structure. It appears to be an edge-on or highly inclined spiral galaxy, or possibly an elliptical galaxy. The central region exhibits a concentrated brightness, suggesting a bulge or a dense core. The overall color profile indicates an older stellar population, as evidenced by the reddish-yellow hue, particularly prominent in the central region. The outer regions seem fainter and less resolved, possibly indicating the presence of a more diffuse disk or halo. There are no apparent signs of significant star formation regions or dust lanes visible in this image, indicating a lower current star formation rate. The galaxy does not show any clear signs of major disturbances or interactions, retaining a largely undisturbed morphology.
