The object appears to be a spiral galaxy, viewed edge-on. The central bulge is prominent and appears relatively large. The disk component is thin and elongated, with a smooth texture. There is a noticeable lack of distinct spiral arm structure visible, likely due to the edge-on orientation and the distance to the object. The color gradient suggests an older stellar population and relatively low star formation. A slight warping of the disk is possibly present. There are no apparent tidal features or major signs of an ongoing merger event. The bulge appears rounded in morphology.
