The galaxy presents as a single, concentrated mass of light, suggesting a high degree of central luminosity. It exhibits a generally elliptical morphology, appearing mostly rounded with a slight deviation towards an elongated shape. The light distribution is relatively smooth and centrally concentrated, which could indicate an older stellar population. I observe a subtle color gradient, with the core appearing slightly more yellow. The outer regions show hints of a more diffuse, bluish hue. There's a minor indication of asymmetry, possibly the presence of a tidal stream or dust lane on one side, but more data is needed for confirmation. Overall, the galaxy's light profile is fairly regular, suggesting a lack of significant ongoing merging activity.
