This galaxy presents as a somewhat diffuse, centrally concentrated system. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outwards from the center, there's a transition to a bluer color, suggesting the presence of younger, hotter stars within its disc. There appears to be no spiral arm structure or bar. The galaxy seems to have a smooth morphology. It could be considered an early type spiral galaxy that has no defined structure, or an elliptical that is more disc shaped. Its light distribution appears fairly even. There are no distinct tidal features or evidence of a major ongoing merger. It shows signs of being an isolated galaxy, as there are no other major galaxies nearby.
