The galaxy appears to be a spiral, viewed nearly edge-on. A prominent dust lane bisects the bright central bulge, obscuring a portion of the galaxy’s light. The bulge exhibits a yellowish hue, potentially indicating an older stellar population. Faint, bluish light extends outwards from the central region, suggesting the presence of a disk. This disk structure appears somewhat irregular and possibly disturbed. There are suggestions of faint, diffuse spiral arms extending outwards from the central regions. There seems to be some tidal disturbance occurring. 
