This galaxy appears to be a spiral galaxy observed at a redshift of approximately 0.12. Its effective radius is around 5 kpc. The galaxy exhibits a prominent central bulge, contributing significantly to its overall luminosity. Surrounding the bulge is a relatively well-defined disk structure. While the image resolution is limited, there is some evidence of spiral arm structure. These arms appear to be somewhat flocculent. Color gradients suggest ongoing star formation. The disk is not seen edge-on, but rather at an angle. A small nearby galaxy is also visible, but does not seem to be in the process of merging.
