The galaxy presents as an elongated, disk-like structure. It appears to be at a significant tilt relative to our line of sight. A central bulge is subtly visible, appearing somewhat diffuse and less prominent compared to the overall galactic disc. The light distribution suggests a relatively smooth profile, possibly indicating a more evolved system, but hints of features and irregularities are present. The color gradient transitions from a central region with slightly redder hues to bluer tones at the outer edges of the disc, possibly indicative of ongoing, albeit moderate, star formation in the outer regions. There is a slight indication of a minor disturbance to the galaxy's overall morphology, as there is a distortion to its shape.
