The galaxy presents as an elongated, cigar-shaped structure. A distinct central bulge is visible, exhibiting a smooth texture and a yellowish hue. The bulge appears brighter than the surrounding galactic disk. A fainter, more diffuse disk extends from the central bulge along the major axis of the galaxy. One end of this extension is more pronounced, with a brighter area featuring a reddish hue. Faint traces of what may be a spiral arm structure are visible in the disk, though the overall morphology appears largely smooth. Possible signs of tidal disruption are present, indicating a possible gravitational interaction with another celestial object. There may be an area of active star formation within it due to a reddish-pink color near the central bulge. Overall, the light distribution suggests a relatively mature system, though not without signs of recent or ongoing dynamic activity.
