The galaxy exhibits a disk-like structure, presenting a somewhat inclined view from our line of sight. A notable feature is a central bulge region, which appears brighter and more concentrated than the surrounding disk. The light from this central region appears more yellow/white, potentially indicating an older stellar population. Surrounding the bulge, a more diffuse disk structure is observed. The disk displays a mottled texture, possibly indicative of spiral arm segments or irregular star formation regions. Patches of bluer light are scattered within the disk, suggesting ongoing star formation. There is some visual irregularity to the shape of the outer regions of the galaxy, including a hint of a tidal tail or disturbance on one edge, though no obvious interacting companion is seen. Overall, the galaxy presents an intermediate morphology, possibly an early-type spiral or a disk galaxy experiencing some form of interaction or disturbance.
