The galaxy presents as an elliptical morphology, appearing elongated with a smooth, diffuse light distribution. The light is concentrated towards the center, showing an apparent bulge. There is a color gradient within the galaxy: the central region exhibits a yellow-orange hue, potentially indicating an older stellar population. Progressing outwards, the colors shift to a bluer-white tinge, hinting at some ongoing star formation. There seems to be some minor disturbance happening within the galaxy, but overall the galaxy shows no obvious signs of major mergers or tidal disruption.
