The galaxy presents a largely smooth morphology, lacking prominent spiral arms or a well-defined disk. The light distribution appears centrally concentrated with a bright, reddish core that fades outwards into a more diffuse halo. The galaxy appears nearly circular or slightly elliptical, with no obvious signs of major tidal disturbances or ongoing mergers, though some minor asymmetries cannot be ruled out. The color profile suggests a population of older stars, particularly in the central region, with hints of ongoing or recent star formation in the outer regions. The galaxy's overall structure implies it is a relatively massive system.
