The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a bright, concentrated luminosity, shifting in color toward the redder end of the spectrum, suggesting an older stellar population and a lack of significant ongoing star formation in this central region. Moving outward from the core, the luminosity gradually decreases. The outer regions appear more diffuse with bluer hues, implying the presence of some younger stars or ongoing star formation, albeit at a seemingly low rate. The galaxy's overall shape is neither perfectly spherical nor highly elongated, tending toward a more intermediate ellipsoidal form. There are no obvious signs of significant tidal interactions or major disturbances in its morphology, indicating it is a relatively settled system. Slight asymmetry may be present but is not significant. The light suggests a galaxy with substantial mass.
