The galaxy presents a relatively smooth and featureless appearance. It exhibits a flattened, disk-like structure seen edge-on. The central region is brighter and appears more concentrated. The galaxy appears to be relatively isolated and does not appear to be undergoing any major merging activity, but some possible minor disturbances may be present. There may be some star formation taking place, likely at a low rate. The overall color of the galaxy suggests an older stellar population. The galaxy appears to be of intermediate size and mass.
