The galaxy presents as a somewhat asymmetric disk-shaped structure with a central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. A faint, broad disk extends outwards from the bulge and appears inclined relative to the line of sight. There is some mottled texture within the disk, possibly indicative of star-forming regions. The outer regions of the disk display a bluer color, potentially signifying the presence of younger, hotter stars. There is a subtle hint of a spiral arm structure on one side of the galaxy, while the opposite side appears more diffuse. Faint irregularities are visible, possibly due to tidal interactions. Overall, the galaxy shows characteristics of an intermediate spiral type with ongoing star formation.
