This galaxy exhibits a distorted morphology, possibly indicative of an ongoing or recent merger event. It appears to be disk-dominated, though with a noticeable central bulge. There is evidence of spiral arm structure, although it is somewhat irregular and disrupted. Color gradients suggest a distribution of stellar populations, with bluer regions possibly corresponding to areas of recent star formation and redder regions associated with older stellar populations. The galaxy's overall shape is elongated and relatively flattened. There is a presence of some dust lanes near its center. The stellar mass is approximately 10^10 solar masses and displays moderate star formation activity.
