The galaxy appears as a moderately luminous, disk-shaped system, observed at an angle that is oblique to our line of sight. Its light profile indicates a centrally concentrated spheroid and a fainter disk component. Some disk features are present, such as spiral arms, but they are largely indistinct. The system lacks any obvious strong signs of recent or ongoing major merger activity, though subtle disturbances in its morphology may indicate a minor interaction. Based on its color and apparent morphology, the galaxy has relatively low ongoing star formation activity.