The galaxy presents as a relatively smooth, elliptical morphology. It exhibits an elongated, cigar-like shape. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer edges. The core region displays a yellowish hue, possibly indicating an older stellar population. Fainter blueish structures are present at the periphery. There is no clear evidence of strong spiral arm structures or a distinct central bulge. The galaxy appears relatively undisturbed, lacking any significant signs of ongoing merger activity or tidal distortions.
