The galaxy presents as a relatively smooth, elongated structure. Its light profile appears concentrated towards the center, suggesting a possible bulge or nucleus. There is a subtle color gradient visible, with the central region exhibiting a slightly warmer hue compared to the outer regions. There are no obvious spiral arms or dust lanes visible in the image; the overall morphology suggests an elliptical type, or possibly a lenticular galaxy viewed close to edge-on. There are no strong indications of ongoing major merger activity, although some minor morphological disturbances cannot be ruled out based on this single image.
