The galaxy appears as a moderately bright object with a generally smooth morphology. It exhibits an elliptical shape, leaning towards an 'in between' classification on the roundness scale, not distinctly circular nor elongated. The light distribution is concentrated towards the center, diminishing gradually outwards, suggesting a higher density of stars and gas in the core. The color gradient transitions from a slightly redder core region to a somewhat bluer outer halo. There is no evidence of strong spiral arms or a prominent disk structure. Marginal signs of tidal disturbance are present, suggestive of a possible past minor interaction or merger event.
