The galaxy presents as a slightly elongated, lenticular structure. It exhibits a prominent, bright central bulge, which appears to be composed of older stellar populations, indicated by the yellowish hue. Surrounding the central bulge, there's a fainter, more diffuse disk. The disk structure appears relatively smooth, lacking significant spiral arm features. The galaxy does not display any obvious signs of a major ongoing merger, though subtle disturbances cannot be entirely ruled out given the image resolution. It presents a low rate of star formation. The size of the galaxy seems moderate for galaxies at its redshift. Overall, it is a typical disk galaxy.
