The galaxy presents as a generally smooth, elliptical object with a notable elongation. It appears to be a relatively undisturbed system, lacking prominent spiral arms or other significant structural features. The light distribution is centrally concentrated. Color gradients are subtle but present; the central region exhibits a bluer hue, suggesting the presence of younger stellar populations, while the outer regions appear slightly redder. There is a hint of mild tidal disruption of the galaxy shape, though no clear evidence of any strong interactions or merger events. The overall impression is that of a galaxy transitioning between a relatively stable state with hints of past or current low-level interaction.
