The galaxy presents as an edge-on spiral system. A prominent dust lane obscures the midplane, creating a distinct dark band across the elongated central bulge. The bulge appears to be centrally concentrated and somewhat rounded. There is some evidence of tidal disturbances, perhaps indicative of past or ongoing interactions. This galaxy also exhibits a distinct merging event. The galaxy displays a subtle color gradient, with the bulge region showing a slightly yellowish hue, potentially indicating an older stellar population. Overall, the galaxy appears to be a relatively massive system undergoing interaction processes.
