The galaxy exhibits a distinct disk morphology, viewed almost perfectly edge-on from our vantage point. The central bulge appears prominent and elongated, displaying a smooth texture. The galaxy's disk shows subtle evidence of internal structure, but is mostly diffuse in appearance. There is a slight indication of a boxy shape to the central bulge, though it appears predominantly rounded. No major signs of ongoing or recent merger activity are apparent. The overall color profile is consistent with a population of older stars.
