The galaxy presents as a relatively thin, elongated structure, suggesting an edge-on or near edge-on disk orientation with respect to our line of sight. A central bulge is evident, appearing bright and concentrated with a yellowish hue, possibly indicative of an older stellar population. The disk component extends outwards from the bulge, displaying a fainter, bluish-white color, consistent with ongoing or recent star formation. The overall shape is relatively smooth with no clear spiral arm structures visible. There is a subtle asymmetry along the disk's length, potentially indicating minor gravitational disturbance or an interaction event.
