The galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. A central bulge is readily apparent, showing a somewhat rounded profile with a yellowish hue. This suggests an older stellar population within the bulge. The disk itself is elongated, with a noticeable dust lane likely obscuring some of the light from the far side of the disk. The disk appears relatively smooth in texture, with a slightly bluer color than the bulge suggesting active star formation, although no distinct spiral arm structures are resolved. There is no obvious evidence of a major merger or significant tidal disturbance affecting the galaxy's overall structure, although subtle asymmetries cannot be ruled out at this resolution.
