The galaxy appears to be a spiral galaxy, presenting with a disk-like morphology. The image reveals the presence of spiral arms, though they are not sharply defined, and appear somewhat patchy. A central bulge is visible, with an intermediate size relative to the overall galaxy. There is some evidence of disturbance, possibly indicative of a minor interaction or past merger event. The colors suggest a mix of stellar populations, with some bluer regions associated with younger, star-forming regions within the spiral arms, and redder hues in the bulge, likely associated with older stellar populations. Overall, this galaxy shows characteristics of ongoing star formation within its disk, coupled with a developed, older bulge component, with some disruption to its morphology.
