The galaxy presents as a primarily disk-shaped structure, viewed edge-on or at a high inclination angle. There is a bright, concentrated central bulge or core region exhibiting a bluish-white color, indicating a high concentration of relatively young, hot stars and active star formation or the presence of an active galactic nucleus (AGN). The disk component shows a yellow-green hue, which likely results from a mix of older stellar populations and dust lanes obscuring some of the bluer light. The presence of redder regions towards the outer edges suggests older stellar populations or dust extinction. The galaxy shows signs of some disturbance, possibly a minor tidal interaction or a past merger event. There is a slight asymmetry to the disk, and faint extensions or distortions may be present. The main body is approximately 5 arcseconds in diameter.
