This galaxy presents as a well-defined, flattened disk structure, viewed nearly edge-on. The central bulge appears small and bright, exhibiting a yellowish-white color, suggesting an older stellar population. The disk is predominantly blue, indicative of ongoing star formation. A dust lane bisects the disk horizontally, appearing as a dark band obscuring the light from the stars behind it. Faint extensions are visible perpendicular to the disk, possibly tidal streams, jets or related to dust scattering from the galaxy. The outer regions of the galaxy have a more diffuse glow, fading into the background. There appears to be a slight asymmetry in the disk. Overall, the galaxy displays characteristics consistent with a spiral or lenticular type. The structure suggests the possibility of a past minor merger event.
