The galaxy presents as an elongated, disk-like structure, viewed at a significant angle relative to its plane. The central region appears brighter and more concentrated, exhibiting a yellowish hue, suggestive of an older stellar population. Moving outwards from the center, there is a gradual decrease in luminosity. Some evidence of faint, bluish tinges can be seen in the outer parts of the disk, especially on the galaxy's edges. There are also small, localized regions of reddish emission within the disk. There is no obvious spiral structure. Overall, the galaxy seems to be relatively undisturbed, showing no signs of a major ongoing merger event, but there may be some signs of minor disturbances. The shape appears more cigar-like.
