The galaxy appears to be a relatively small, elongated system, presenting an edge-on or highly inclined disk morphology. The central bulge is not prominently visible, suggesting a disk-dominated structure. The light distribution is smooth, with no obvious spiral arm features or irregular clumps of star formation visible in this image. The color is consistent with a galaxy comprised primarily of aging stellar populations. There are no signs of significant tidal disturbances or ongoing merger activity, although subtle distortions or a faint stellar halo cannot be ruled out with this image resolution. The lack of strong color gradients or distinct structures suggests a relatively quiescent galaxy, possibly in a transition phase.
