The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology suggests it is likely an elliptical galaxy. The light distribution is fairly symmetrical. There is no obvious spiral structure or bar. The object appears a golden yellow hue which likely indicates an older stellar population. The galaxy appears fairly isolated, with no signs of major tidal disturbances or ongoing mergers. There may be a very slight extension of the galaxy's light along one axis, hinting at a possible minor interaction or subtle deviation from perfect elliptical symmetry. The object exhibits a high degree of central concentration, with the intensity decreasing gradually towards the outer regions.
