The galaxy presents as a smooth, elliptical-like structure. The central bulge appears prominent and exhibits a concentrated luminosity, suggesting a high density of stars. The galaxy's color profile indicates an older stellar population, with the dominant hues leaning towards the redder end of the spectrum, possibly indicative of less active star formation. The outer regions of the galaxy gradually fade into the background, lacking distinct spiral arm features or significant dust lanes, which further supports its classification as an elliptical galaxy. The overall shape deviates slightly from perfectly circular, hinting at a degree of ellipticity. There are no obvious signs of major tidal disturbances or ongoing mergers in this image, though some slight asymmetries in the outer halo might suggest minor interactions or past gravitational influences.
