This galaxy appears to be a spiral galaxy, viewed edge-on. A prominent dust lane bisects the galaxy, obscuring the central bulge. The galaxy exhibits a relatively smooth disk. The stellar population seems diverse, with hints of younger, bluer stars interspersed with older, redder populations. There is a faint indication of a possible tidal stream or minor disturbance in the galaxy's halo, suggesting a past or ongoing interaction with a smaller companion, but it is not a major merger. The disk itself is elongated and appears to be relatively thin. The overall color indicates ongoing star formation, although at a moderate rate. There is no clear presence of a massive, actively accreting supermassive black hole, as the galaxy does not appear to have a bright, point-like nucleus or a jet.
