The galaxy exhibits a distinct disk-like morphology, oriented at an oblique angle relative to the observer. Spiral arm structures are apparent throughout the galactic disk, with two main arms observed. The spiral arms appear relatively tightly wound and extend outwards from the central bulge region. The central bulge is moderately sized, appearing neither dominant nor negligible in comparison to the disk. There's a suggestion of a bar-like structure crossing the central region of the galaxy. Star formation appears to be actively occurring within the spiral arms, as evidenced by the slightly enhanced blue color within these regions compared to the more yellow/red central regions. No major tidal disturbances or signs of significant recent merger events are clearly discernible. The galaxy appears as a well-formed, relatively undisturbed spiral system.
