This galaxy exhibits an irregular morphology. The light distribution appears somewhat smooth, but also shows evidence of disturbed structure, potentially indicative of ongoing or recent interactions. The overall shape can be described as somewhere between round and cigar-shaped. There is a hint of possible tidal features or faint extensions, suggesting potential gravitational interactions with nearby galaxies, possibly even merging. The presence of these irregular features supports the possibility of mergers, minor disturbance, or major disturbance within this galaxy. There appear to be regions of differing stellar populations, evidenced by the varying colors, indicating differing levels of star formation activity. Some regions appear bluer, indicative of ongoing star formation, while others appear redder, signifying older stellar populations. 
