The galaxy presents as a lenticular or spiral galaxy seen edge-on. A prominent central bulge is visible, appearing generally rounded in shape. The disk component is elongated and thin, exhibiting a relatively smooth texture with no clear evidence of spiral arm structure or prominent dust lanes in this image. The color gradient suggests a potentially older stellar population dominating the bulge, indicated by the yellowish or orange hue, while the disk appears somewhat bluer, implying ongoing, low levels of star formation. There is no apparent significant interaction with other galaxies or any major morphological disturbances to suggest a recent merger event. Overall, it appears as a relatively isolated, well-formed disk galaxy at a moderate redshift.
