This galaxy exhibits a generally disk-like morphology, although the structure appears somewhat irregular. There is a bright, concentrated central region. The overall color is bluish-white, suggesting a population of relatively young stars. There are hints of spiral arm structure in the outer regions, but they are not well-defined. There appears to be some form of minor disturbance or interaction occurring, based on subtle asymmetries in the shape and light distribution. There is also evidence of potential merging features within the galaxy, but they are not prominently visible. Overall, this object displays characteristics indicative of both a disk galaxy and a possible interaction or minor merger event.
