The galaxy appears to be a spiral type, viewed at a high inclination, likely nearly edge-on. The major axis is oriented approximately along the northeast-southwest direction. The central bulge is not prominent, blending into the overall structure. There is some indication of a disk structure, with hints of dust lanes visible along the plane of the galaxy. Faint blue regions are visible, potentially indicative of star formation. The galaxy’s overall morphology appears somewhat disturbed, potentially indicating a minor interaction or merger event in its past. There may be a slight tidal feature extending outward from the main body of the galaxy.
