The galaxy presents as a somewhat smooth, elongated structure with a high degree of ellipticity. A subtle color gradient is visible, with a central region appearing more yellowish-white, possibly indicating an older stellar population. Fainter blue regions are seen further from the core, suggesting a small degree of on-going star formation. There is no distinct nucleus and the edges appear diffuse. Overall, the galaxy's morphology is consistent with that of a spiral galaxy viewed edge-on or an elliptical galaxy. There are no obvious signs of tidal disturbances or a major merger event, and the galaxy appears relatively isolated in this field of view.
