The galaxy presents as an edge-on spiral, exhibiting a prominent, centrally located bulge that appears relatively smooth and rounded. This central region displays a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer light extends outward from either side of the bulge, implying the presence of a disk structure and the potential for ongoing star formation activity in the arms. The disk appears relatively thin and uniform, with only subtle variations in brightness along its length. There is no clear evidence of any major merger events or strong tidal disturbances, although subtle asymmetries in the disk's structure might indicate minor interactions. Overall, the galaxy exhibits a morphology consistent with a spiral galaxy undergoing a moderate degree of star formation.
