The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing mostly in between round and cigar shaped. There is a hint of possible minor disturbance in the galaxy's overall structure, but no conclusive signs of merging activity are observed. Color gradients are subtle, with a slightly bluer hue towards the central regions, suggesting the presence of younger stellar populations or ongoing star formation. The galaxy displays no apparent spiral arm structures.
