The galaxy appears as a somewhat symmetrical, though not perfectly circular, object. It presents a generally smooth morphology, showing little evidence of significant spiral arm structures or large-scale irregularities upon visual inspection. The core region seems more concentrated and brighter than the outer regions. The color profile appears somewhat homogenous across the galaxy, with a slight shift toward redder hues as opposed to a strong blue color. There is no evidence of any major ongoing merger events, strong tidal tails or strong distortions in its form. This suggests that the galaxy is relatively undisturbed at this point in time.
