The galaxy appears to be a relatively small, edge-on or highly inclined spiral, possibly disk-shaped. The central bulge is not very prominent. The galaxy exhibits a smooth morphology, with a hint of a disk structure and some possible internal features. The galaxy has a slightly elongated appearance, consistent with it being viewed at an angle. There may be some active star formation regions, observable as slightly bluer patches. Overall, the color suggests a mix of stellar populations, with some younger stars and some older stellar populations. There appears to be very little disturbance of the structure and no signs of any on-going major merger events.
