The galaxy presents as a somewhat flattened spheroid, appearing as a disk galaxy viewed at a moderate inclination. The central bulge exhibits a bright, yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the disk displays a bluer tint. A fraction of the galaxy shows faint signs of disturbance or perhaps minor tidal interactions. No strong spiral arm structures are distinctly visible. The overall form suggests an intermediate type between a pure elliptical and a well-defined spiral, but leans slightly towards the smooth, elliptical morphology, with no dominant features. The galaxy is a significant mass with relatively low ongoing star formation. It is exhibiting properties intermediate between active and passive star formation, as well as star formation that is likely nearing its end.
