The galaxy presents as a relatively smooth, disk-shaped structure seen nearly edge-on. The central bulge appears prominent and exhibits a yellowish-white hue, suggesting an older stellar population. The disk is elongated, with a high degree of ellipticity. There is no discernible spiral arm structure or evidence of active star formation regions within the disk based on the image. The galaxy displays a moderate redshift, indicating a relatively distant object. The overall appearance suggests a galaxy dominated by older stars, with potentially minimal ongoing star formation. There might be signs of minor disturbances in the outer regions of the disk, but not significant enough to categorize this as a major merger event.
