The galaxy presents a generally smooth morphology. Its shape is highly elongated, appearing cigar-shaped with a significant axis ratio. There is no obvious bulge structure. The color gradient transitions from a redder hue at the core to slightly bluer tones towards the outer edges, possibly indicating some ongoing star formation in the disk. There appears to be no strong indication of spiral arm structures or a prominent dust lane. No significant tidal disturbances or signs of a major merger event are apparent, though some minor disturbance cannot be ruled out due to image quality and perspective.