The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. There is a slight deviation from perfect sphericity, tending towards an intermediate elliptical shape. A concentrated bulge dominates the galaxy's center, exhibiting a bright, almost stellar-like core. The overall color profile suggests a relatively passive stellar population, leaning towards redder wavelengths, although some bluer regions are discernable indicating the presence of recent star formation. Subtle disturbances or asymmetries are visible in the galaxy's outer regions. Given these features, it's possible we're observing a galaxy that may have experienced minor merger activity in its recent history.
