The galaxy presents an elongated, cigar-shaped morphology. Its overall color suggests a mix of stellar populations, with a central concentration exhibiting a yellowish-orange hue, potentially indicating an older stellar population or a significant dust component. Extending outward from the central region, a fainter, bluish component is visible, indicative of possible star formation activity within a disk-like structure. There is some distortion visible at the lower edge of the galaxy. The galaxy appears relatively smooth in texture, with some minor irregularities possibly suggesting a minor interaction or internal disturbance.
