The object appears to be a spiral galaxy, viewed nearly edge-on. A prominent central bulge is observed with a yellowish-orange hue, suggesting an older stellar population with relatively little ongoing star formation. The disk of the galaxy, oriented vertically, is elongated and appears relatively smooth, with only subtle indications of spiral arm structure. The galaxy exhibits a relatively faint blueish tint along the edges of the disk, possibly indicating regions of recent star formation. The overall morphology suggests a substantial disk component and a dominant bulge, which may indicate that it is a late-type spiral galaxy. The high inclination angle makes it difficult to assess the presence of bar features or other internal structures. There is no evidence of major mergers or strong tidal disturbances from this image alone.
