The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region indicative of a prominent galactic nucleus. The morphology appears largely undisturbed, lacking any obvious signs of tidal tails, strong asymmetries, or major merger events. There's a slight elongation present in the galaxy's shape, hinting towards a deviation from perfect sphericity. The color profile suggests the presence of both older stellar populations, indicated by the redder hues, and a component of ongoing or recent star formation, as evidenced by the bluish tints, particularly in the central region. The overall luminosity suggests a galaxy of substantial stellar mass. The lack of well-defined spiral arms or a distinct disk component further supports the classification as an early-type galaxy.
