The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The central region exhibits a yellowish-white hue, indicative of an older stellar population. A faint, diffuse blue region is apparent on one side, suggesting the presence of a region of more recent star formation. Overall, the galaxy appears fairly undisturbed with no obvious signs of major mergers or tidal features, however some minor distortions in its form may indicate past gravitational interaction.
