The galaxy presents as a spiral galaxy with a disk-like structure viewed at an oblique angle. A defined central bulge is visible, exhibiting a moderate size relative to the disk. The spiral arms are prominent and well-defined with two clear arms emanating from the central region. The winding of the arms appears somewhat loose, suggesting a less tightly wound spiral pattern. The overall color distribution indicates regions of both older stellar populations in the central bulge and ongoing star formation within the spiral arms, as evidenced by the bluer hues. There may be minor disturbances or irregularities in the disk, which could be indicative of past or ongoing interactions with another galaxy or gravitational influences. The overall appearance suggests a galaxy that is not currently undergoing a major merger, though some level of interaction cannot be ruled out.
