The galaxy appears as an elongated, somewhat cigar-shaped structure. It exhibits a relatively smooth overall appearance. There is a central bulge that is bright and concentrated, transitioning to a less bright, more diffuse disk component. The disk has a blue hue, which may indicate active star formation. There is no evidence of strong spiral arm structure or major disturbances in the galaxy's morphology, although some minor irregularities can be observed, perhaps indicating minor interactions. The overall profile suggests the galaxy is an edge-on or highly inclined spiral, or possibly an elliptical galaxy with a flattened shape. 
