The observed galaxy presents an irregular morphology. It does not exhibit a clear spiral arm structure or elliptical symmetry. The light distribution is somewhat clumpy, suggesting possible active star formation regions or tidal disturbances. There appears to be a primary concentration of light, but it is not centrally condensed, and the overall light profile shows no apparent bulge. The colors present across the galaxy appear to show variation. In one region, a yellow hue dominates, and then moves into a redder hue. This could potentially indicate variations in stellar populations and dust content within the galaxy. There might be ongoing interactions or merger events occurring.
