The galaxy presents as a spiral structure, with a notable disk component exhibiting distinct spiral arms. The arms appear relatively well-defined and traced by regions of brighter, possibly younger, stellar populations. The winding of the arms suggests an intermediate morphology, neither tightly wound nor overly loose. A bar feature appears to be present within the central region, extending through the bulge. The bulge itself is moderately sized relative to the disk. Overall, the galaxy does not appear to exhibit significant signs of ongoing major merger activity; however, some minor distortions or peculiarities in the disk morphology cannot be ruled out. The light distribution suggests a substantial fraction of star formation. The estimated size of the galaxy is a few kiloparsecs in radius. The galaxy is at redshift z~0.1.