The galaxy presents as a single, relatively featureless object. The light distribution appears smooth and centrally concentrated. It exhibits an elliptical morphology, tending towards a cigar shape, with its major axis oriented approximately vertically in the frame. There is no evidence of a distinct nucleus or spiral arm structure. Some minor perturbations may be present, however the majority of the light appears to be distributed in a smooth, continuous fashion. The color gradient suggests some difference in stellar population or dust content, with a slightly bluer hue towards the center and redder extending outward. However, these color variations are subtle.
