The observed galaxy exhibits a distinct disk morphology, appearing nearly edge-on from our vantage point. The central bulge is prominent, presenting a rounded appearance. A dark dust lane bisects the galaxy along its major axis, obscuring some of the light from the bulge. This obscuration suggests the presence of significant interstellar dust and gas within the galactic plane. The disk shows some evidence of features or possibly spiral structure, but the limited resolution and edge-on orientation makes these features difficult to categorize with certainty.

Overall, the galaxy's light appears reddened, particularly near the galactic center, which is consistent with dust extinction. There does not appear to be any major disturbances to its overall structure, yet some irregularities exist in the outer disk, suggesting the possibility of past or ongoing minor interactions. There is no evidence to support the presence of a significant or ongoing merger.