The galaxy presents as a slightly elliptical, disk-like structure. There is a noticeable bulge component, appearing brighter and more concentrated towards the center. The bulge exhibits a yellowish-orange hue, which could suggest an older stellar population. The disk component appears fainter and somewhat bluer than the bulge, hinting at ongoing or recent star formation. The disk appears relatively smooth, lacking prominent spiral arm structures that are readily discernible. Faint, diffuse light extends beyond the main body of the galaxy, indicating the presence of an extended halo or tidal features. There might be some minor disturbances or interaction indicated by the fuzziness of the outer edges. Overall, the galaxy displays a morphology intermediate between a pure elliptical and a well-defined spiral.
