The galaxy appears to be a spiral galaxy viewed nearly edge-on. There is a concentrated central bulge that appears relatively smooth and bright with a blue hue. Fainter regions of the galactic disk extend from the central bulge along a generally horizontal axis and give it an overall oblate appearance. There is not much discernible structure, such as well-defined spiral arms, suggesting it might be a late-type spiral. The disk appears relatively smooth. The light is somewhat blue, indicating ongoing star formation. There is no evidence of tidal tails or disturbed morphology, suggesting no major merger events are presently occurring, though some minor disturbances are possible. The galaxy appears to be relatively isolated.
