The galaxy exhibits a disk-like morphology, with an estimated physical half-light radius of approximately 8.5 kpc. The disk is presented nearly edge-on to our line of sight. A central bulge component is observed, appearing relatively smooth and concentrated. Evidence of internal structure, potentially spiral arms or dust lanes, are visible, although partially obscured by the edge-on orientation. Irregular features and disturbances suggest a possible interaction or minor merger event. The galaxy displays varying colors, with the central bulge tending towards a yellow-red hue, indicative of an older stellar population, while bluer regions suggest ongoing star formation within the disk.
