The galaxy presents as an elongated, cigar-shaped structure. It appears to be a disk galaxy observed at a significant angle to our line of sight. A central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. There is a subtle color gradient observed across the galactic disc, the outer regions of which have a bluish tint, suggesting the presence of younger, hotter stars. There is no clear spiral structure visible in the galaxy. There is a slight irregularity in the shape of the disk, but no signs of a major ongoing merger.
