The galaxy presents as a spiral type, exhibiting a prominent disk structure. The disk is not perfectly edge-on, showing some inclination relative to our line of sight. Spiral arms are visible, and appear relatively tightly wound. A central bulge is present, appearing moderately sized and exhibiting a bright core. The overall color suggests active star formation, with a discernible bluer hue in the disk and arms. No strong bar feature is apparent. There is a slight asymmetrical appearance to the galaxy, with a possible minor disturbance suggesting an interaction with another galaxy or recent merger event. The galaxy displays both smooth components, possibly indicating an older stellar population, along with more featured components of a star forming disk and spiral arms.
