The galaxy presents a generally smooth morphology. There is evidence of a central bulge, with a gradient of light intensity outwards from the core. The ellipticity suggests that this is not a face-on spiral, rather an elliptical, or perhaps a spiral with a substantial inclination. The color profile suggests that it is likely composed of an older stellar population. The galaxy displays no obvious signs of active merging activity, though there may be slight asymmetries. It exhibits characteristics consistent with a lenticular type galaxy. There appears to be evidence of ongoing, albeit potentially low, levels of star formation, which could suggest that the galaxy is in the process of quenching or may be undergoing a minor rejuvenating event. Its overall mass appears to be relatively high.
