The galaxy presents as an elongated structure, likely a disk galaxy viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. The bulge appears largely rounded in shape. Emanating from the central bulge is a diffuse, bluish disk. The blue color hints at the presence of younger, hotter stars indicative of ongoing or recent star formation within the disk. There appears to be noticeable dust lanes present within the disk of the galaxy. The galaxy displays some irregularities in its structure, suggesting possible gravitational interactions or minor disturbances. These could be indicative of tidal effects from a previous interaction or ongoing minor merger events. The overall morphology suggests a galaxy undergoing active evolutionary processes.
