The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a prominent, bright central bulge that fades gradually into a disk. The bulge appears largely featureless and concentrated. The disk is moderately inclined relative to our line of sight, imparting an elliptical appearance. The light distribution shows a smooth profile indicating an evolved stellar population. Faint spiral arm structures are faintly suggested in the disk, but ill-defined and patchy, with what appears to be a small section on one side appearing as blue, indicating relatively active star formation on that side. The outer regions of the disk fade into the background sky, with no obvious signs of truncation or interaction. The color gradient suggests that star formation has largely ceased throughout the galaxy, except the single patch on the disk that exhibits a slightly bluer hue indicating a region of younger, hotter stars, therefore ongoing active star formation. Overall, this appears to be a relatively massive galaxy at a moderate redshift.
