The galaxy presents an elongated, disk-like morphology with a prominent central bulge. The core exhibits a concentrated brightness, suggesting a high stellar density in this region. The disk shows hints of spiral arm structure but appears somewhat irregular or disturbed. Patches of bluer light are observed, possibly indicative of ongoing star formation regions within the disk. A possible tidal tail or disturbed companion galaxy is present on one side of the primary galaxy. The overall color index suggests an intermediate-age stellar population with evidence of both recent star formation and older, more evolved stars. The galaxy shows signs of interaction or merging.
