The galaxy presents as a somewhat diffuse, centrally concentrated object. The overall morphology appears relatively smooth. The galaxy does not exhibit strong spiral arm structures, and the light appears to be primarily emanating from the central region. There is some indication of bluer emission in the center, suggesting some ongoing star formation. The galaxy appears to be in a relatively unperturbed state. There is a slight elongation. The galaxy shows a gradient in color, with the central region appearing bluer and becoming redder in the outer regions.