The galaxy presents as a moderately bright object with a slightly elongated morphology. There appears to be a primary central body which is relatively smooth in appearance. There is evidence of a possible secondary component on the right of the primary structure. The galaxy exhibits a color gradient, transitioning from a more yellow-white hue in the center to bluer tones in the outer regions and particularly concentrated within the secondary component. Faint extensions might be present, though the contrast is low. There are possible disturbances in the overall symmetry of the structure. The overall impression suggests a possible interaction or merger event, given the non-uniform shape and color distribution.
