The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, diffuse light distribution, suggesting a relatively homogeneous stellar population. There is a slight color gradient observable, with a somewhat bluer hue towards what appears to be the outer regions and a more yellowish tinge centrally. The overall structure lacks prominent spiral arms or distinct features. While there is a hint of asymmetry, no clear signs of a recent major merger or tidal disturbances are apparent. The light profile diminishes gradually from the central core outwards, with no sharp cut-off.
