The galaxy exhibits a spiral morphology, presenting clear evidence of spiral arm structures. These arms appear somewhat flocculent rather than tightly wound. The disk component is dominant, with a relatively small or negligible bulge. Blue hues are prominent, indicating a significant population of young, hot stars and ongoing star formation. The galaxy shows signs of interaction or merging activity, as there are some disturbances within the overall structure. It is not edge on. The galaxy appears relatively isolated. There is some evidence of a bar structure. The overall impression is of a moderately sized, actively star-forming spiral galaxy undergoing some level of disturbance, possibly due to a minor merger.