The galaxy presents as a slightly elliptical, disk-like structure, inclined at a shallow angle to our line of sight. A central bulge is discernible, appearing smooth and concentrated. The overall color profile suggests a mix of stellar populations, with a subtle bluer hue throughout the galactic disk, possibly indicating ongoing or recent star formation. The disk displays some signs of disturbance, although no distinct spiral arms are readily apparent, and there are no clear signs of a major merger in progress, such as tidal tails or strong asymmetries. The galaxy's general morphology suggests it is likely transitioning from a more active star-forming phase to a state of relative quiescence.
