The galaxy presents as an elongated, cigar-shaped morphology, likely an edge-on spiral or lenticular galaxy. A central bulge is visible, exhibiting a yellowish hue suggestive of an older stellar population. The disk, extending outwards from the bulge, shows a bluer color, potentially indicating ongoing star formation. There is a slight hint of asymmetry or a minor disturbance in the outer regions of the disk, particularly noticeable on one side, which might point to past interactions or mergers. Overall, the galaxy appears relatively smooth in structure, with a moderate amount of star formation, suggesting a transition phase in its evolutionary history.
