The galaxy appears to be a spiral type, albeit with a somewhat disrupted morphology. There are hints of faint spiral arms, but they are not well-defined, indicating a possible interaction or disturbance in its past. The central bulge is not particularly prominent; it is not bright and appears relatively small in comparison to the overall size of the galaxy. There is some bluer light emanating from regions within the galaxy, suggesting ongoing, although perhaps not vigorous, star formation. There also appear to be tidal tails or faint streams of stars extending outward from the main body of the galaxy, especially toward the north, which could further support the possibility of a past merger or gravitational interaction with another galaxy.
