The galaxy presents as an elliptical-like structure. It exhibits a generally smooth morphology, with a high degree of central concentration. The galaxy displays a moderately high degree of roundness in its overall shape, though it appears not perfectly circular. The color profile suggest a intermediate age stellar population. There is no strong evidence of spiral arm structures or significant dust lanes. There does not appear to be evidence of ongoing major mergers or significant tidal disturbances in the immediate vicinity of the galaxy. Overall, this galaxy appears to be a relatively undisturbed elliptical, likely in a relatively stable state of evolution.
