The galaxy presents a discernible disk structure with indications of spiral arms. A bar-like feature is present within the central region, exhibiting a notable axis of symmetry. The bulge component appears moderate in size relative to the disk. The galaxy does not show obvious signs of a major merger event, but the morphology suggests the possibility of minor disturbances or interactions. The galaxy displays a mix of stellar populations, evidenced by varying color gradients within its structure. It is likely a spiral galaxy exhibiting a barred morphology and moderate bulge prominence, with potential signs of past or ongoing interactions influencing its structure.
