The galaxy appears to be a lenticular or possibly a spiral galaxy viewed at a high inclination. A bright, yellowish region is visible at one end, possibly representing an older stellar population. The main body of the galaxy exhibits a bluer hue, suggesting the presence of ongoing star formation. A slight curvature is visible, indicating some disk structure. There is a suggestion of a faint tidal tail or disruption on one side, perhaps indicating an ongoing or recent merger event. Overall, the galaxy displays a morphology that falls between smooth and displaying features. The galaxy does not exhibit a clear, dominant bulge.
