The galaxy presents a clear disk morphology, viewed edge-on from our perspective. A prominent central bulge is observed, appearing concentrated and yellowish in color, suggesting a population of older stars. Fainter disk light extends away from the bulge on either side, with a blueish tint that becomes more dominant further from the core, potentially indicating a more recent and ongoing star formation. The disk light appears to taper at the edges, with some mottling suggesting possible dust lanes or clumps of star formation. The overall structure is elongated, exhibiting a high degree of flattening.
