The galaxy presents a complex morphology. It appears to be a spiral galaxy, exhibiting well-defined spiral arms. The arms appear somewhat clumpy, indicating active star formation regions within them. The central bulge is prominent but not overwhelmingly dominant, displaying a moderate size. The galaxy's disk is viewed at an angle that is not precisely face-on, but not quite edge-on. There are indications of potential minor disturbances or ongoing interactions, potentially even a merger event, given the somewhat irregular appearance of the spiral arms. The galaxy displays colors consistent with a population of both older stars and more recently formed, hot stars within the spiral arms.
