The galaxy presents as a lenticular or possibly an elliptical system, characterized by a smooth, elongated morphology. It is significantly more extended along one axis, indicating a cigar-like shape. The primary body of the galaxy exhibits a yellowish hue, suggesting an older stellar population and a relative paucity of ongoing star formation. A notable feature is a smaller, bluer region situated on one side of the main galactic disk or spheroid, which potentially indicates a region of more recent star formation or a separate, gravitationally interacting object. There are no apparent signs of major mergers or significant tidal disturbances.
