The galaxy presents an elongated, cigar-shaped morphology. Its central region exhibits a high degree of luminosity, suggesting a concentrated distribution of stars, likely an older stellar population given the yellowish-orange hue. The luminosity gradually decreases toward the outer regions of the galaxy. There appears to be minimal evidence of spiral arm structure or active star formation regions; instead, the galaxy appears smooth and relatively featureless. A subtle color gradient is visible, transitioning from a more reddish tone at its lower end to a slightly yellower tone towards the center. There are no clear signs of ongoing major mergers, though there may be slight asymmetry suggestive of a minor disturbance or tidal interaction. Overall, the galaxy's morphology is consistent with that of an elliptical or lenticular galaxy, viewed edge-on.
