The galaxy appears as a moderately inclined disk system, approximately 8.7 kpc in effective radius. The central bulge exhibits a smooth, yellowish profile, suggesting an older stellar population. Extending from the central region is a fainter, bluer disk structure, indicative of ongoing star formation. There are subtle hints of spiral arm features within the disk, although the resolution is limited. No major disturbances or merger events are readily apparent in the galaxy's morphology, suggesting a relatively undisturbed evolutionary history. The galaxy appears to be of intermediate mass and exhibits a moderate rate of star formation. Overall, the galaxy presents as a typical disk galaxy at a redshift of approximately 0.127.
