The galaxy presents an elongated morphology, appearing as a flattened disk seen at a significant angle to our line of sight. The central region exhibits a brighter, more concentrated luminosity profile, suggesting the presence of a central bulge. The color distribution shows a subtle gradient, with the central bulge appearing slightly more yellow in color, and the outer disk exhibiting a blue hue. This color difference may indicate variations in stellar populations, with the bulge potentially composed of older, redder stars, and the disk containing younger, bluer stars engaged in active star formation. The edges of the disk appear somewhat indistinct, lacking sharp definition, possibly due to dust obscuration or the presence of faint, extended stellar populations in the galactic halo. There are some signs of a tidal disturbance.
