The galaxy presents a mostly smooth morphology, characterized by a dominant central bulge. The bulge appears roughly spherical and exhibits a concentrated luminosity profile, suggesting a relatively old stellar population. Faint discal structures are discernible, oriented in an edge-on formation. The disk appears thin and elongated, indicating that we are observing it at a high inclination angle. There seems to be a minor disturbance in the disk, implying that the galaxy has undergone a potential interaction with a smaller neighboring galaxy. The galaxy appears to be a spiral, but appears to be rather round and undisturbed. The galaxy does not appear to be undergoing any major mergers, but the possibility of a minor merger cannot be ruled out. Based on these observations, the galaxy is likely a spiral galaxy that has been interacting with another, smaller galaxy. The galaxy has a relatively old stellar population, but the presence of faint discal structures suggests that the galaxy is still actively forming stars, albeit at a low rate.
