The galaxy presents as an edge-on or highly inclined disk galaxy, elongated with a length of roughly twice its width. The galaxy appears moderately bright with a concentrated central bulge that exhibits a bluish-white color. Diffuse light is observed extending outwards from the center, suggesting a spiral disk. The disk shows a general overall bluer hue, indicative of ongoing star formation. The outer regions of the disk appear faint, possibly due to dust obscuration or a lower density of stars. There is no obvious evidence of active galactic nuclei or strong tidal disturbances and there is no clearly observed spiral arm structure.
