The galaxy presents a relatively smooth and centrally concentrated morphology, with a noticeable absence of well-defined spiral arms or a prominent bar structure. The light distribution appears diffuse, suggesting a relatively old stellar population. There is a slight bluing color present, potentially indicative of some low-level recent star formation. Its visual shape is somewhat oblong, but without any clear signs of ongoing major merger activity. It is also unlikely to be an edge-on disk. The general appearance points towards an intermediate to massive galaxy with potentially some minor disturbances.
