The galaxy appears to be a spiral, viewed at a high inclination. The central bulge is bright and elongated, exhibiting a yellow-orange hue, potentially indicative of an older stellar population. The disk surrounding the bulge displays blue-ish tinges, suggesting the presence of younger, hotter stars and ongoing star formation. There are hints of disturbed morphology, with some asymmetry in the disk, and possibly signs of tidal interactions. The galaxy shows evidence of a possible interaction or merger, possibly with the secondary object nearby, which may be a smaller galaxy or a tidal dwarf galaxy. The overall structure is moderately disturbed.
