The galaxy presents as an elongated, cigar-shaped structure. Its central region exhibits a brighter, more concentrated luminosity. Surrounding this central hub, we observe a diffuse, greenish-yellow glow that appears to extend along the major axis of the galaxy. The outer regions display a fainter, reddish hue, suggesting a difference in stellar populations or dust content compared to the central region. There is no clear evidence of well-defined spiral arms or a prominent disk. The overall morphology suggests a relatively smooth distribution of light, with no significant signs of ongoing major merger events or tidal disruptions. There appears to be a slight distortion in the galaxy's shape, leading to the cigar shape.
