The galaxy presents a largely elliptical morphology, appearing smooth and relatively featureless. There's a high degree of central concentration, with luminosity peaking at the galaxy's core. The color profile suggests a dominant population of older stars, likely with a low star formation rate. There is a slight elongation, hinting that it may not be perfectly spherical, but rather a slightly flattened spheroid. No spiral arms or significant dust lanes are readily apparent. The galaxy doesn't appear to be undergoing any major mergers or experiencing significant tidal disturbances.
