The galaxy presents as an elongated, disk-shaped structure with a noticeable central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population with lower rates of star formation. Extending outward from the bulge, the disk shows a bluer color, indicative of younger, hotter stars and ongoing star formation. There is an apparent lack of distinct spiral arm structure, giving the galaxy a relatively smooth appearance. The outer edges of the disk appear somewhat diffuse and irregular, possibly due to tidal interactions or the presence of dust lanes. The high axial ratio suggests a near edge-on orientation relative to our line of sight. The overall morphology hints at a late-type spiral galaxy or possibly an early-type lenticular galaxy.
