The galaxy appears as a luminous, elliptical object with a relatively smooth and centrally concentrated light distribution. The core region exhibits a distinct yellowish-white hue, suggesting a population of older stars. The outer regions display a faint, blueish halo which may be indicative of younger stellar populations or ongoing star formation within the galaxy. While appearing largely undisturbed, there is a slight asymmetry visible in the halo. The galaxy appears to have a significant stellar mass, which would correlate to it's notable luminosity. Based on the data, the galaxy appears to be a late-stage galaxy that is no longer forming many new stars.
