The galaxy presents an elliptical morphology, appearing as a relatively smooth, elongated spheroid. The light distribution reveals a central concentration, brightest at the core, with a gradual decline in luminosity towards the outer regions. The color profile seems to shift from slightly redder hues at the core to marginally bluer tones at the outer edges. There may be some minor disturbances happening, as a small irregularity is visible along one edge, but nothing too drastic. Overall, the galaxy seems to be relatively isolated, with no major signs of ongoing merger activity.
