The galaxy presents as a relatively smooth and rounded structure, with a noticeable concentration of light towards the central region. There is a subtle color gradient, shifting from a slightly bluer hue in the outer regions to a redder, yellower core. While the overall shape is generally elliptical, some subtle irregularities or minor disturbances might be present upon closer inspection. The galaxy appears to be in a relatively isolated environment, with no immediately obvious signs of major ongoing mergers or tidal interactions with other galaxies. The light profile suggests a mature stellar population with a moderate amount of ongoing star formation.
