The galaxy presents as a generally smooth object, suggesting it is likely an elliptical galaxy or a spiral galaxy viewed face-on with a dominant bulge. The galaxy exhibits a concentrated central region with a gradual decrease in luminosity outwards. The color profile is predominantly yellow/orange, indicative of an older stellar population with fewer young, massive stars. There is a subtle suggestion of disturbance to the morphology, which could be interpreted as a tidal tail or sign of a minor merger.
