The galaxy presents as a somewhat faint, elongated object. It appears to be a disk galaxy viewed nearly edge-on, as indicated by its needle-like shape. The central bulge is not prominently defined, exhibiting a rather smooth and diffuse luminosity profile. The disk shows subtle hints of internal structure but lacks clearly defined spiral arms, suggesting a relatively smooth distribution of stellar populations. The bluer hue indicates the potential presence of younger, hotter stars and ongoing star formation. The overall morphology suggests a galaxy that is relatively undisturbed, with no signs of major mergers or tidal interactions. Its structure is fairly regular and symmetrical.
