The galaxy presents as a somewhat elliptical structure, with a high degree of central concentration, potentially indicative of a significant bulge component. The galaxy exhibits a smooth appearance, suggesting a lack of prominent spiral arms or distinct morphological features. Color gradients are apparent, with a central region exhibiting a yellowish hue, likely indicative of an older stellar population, while the outer regions appear slightly bluer, suggesting the presence of a younger stellar population, but with a slight amount of dust extinction apparent. There may be a slight warping of one side of the galaxy, implying a possible gravitational interaction with another celestial body.
