The galaxy presents as a relatively smooth, elongated structure with a cigar-like shape. It displays a central concentration of light that appears yellowish-white, suggesting an older stellar population. Fainter, bluish regions are present at the edges of the disk, indicating regions of possible ongoing or recent star formation. There are no apparent signs of major disturbances or tidal features, implying that the galaxy is currently not undergoing a major merger event, however there is a slight asymmetry. The overall morphology suggests a disk galaxy, likely seen edge-on or at a high inclination angle.
