The galaxy presents as a flattened, disk-shaped structure viewed nearly edge-on. A prominent central bulge is observed, displaying a smooth, symmetrical profile. The disk component appears relatively thin and exhibits a pale hue, indicative of an older stellar population. There is no significant dust lane or distinct spiral arm structure visible in this image. The overall morphology suggests the galaxy is an early-type spiral or lenticular galaxy. There are also no nearby galaxies which would imply a merger event or tidal disturbances.
