The galaxy presents a complex morphology, suggestive of an ongoing or recent merger event. A distorted, luminous central bulge is visible, exhibiting a relatively smooth texture. A prominent tidal feature arcs away from the main body, indicating significant gravitational interaction. The disk is clearly disrupted, with asymmetric spiral arm fragments visible, suggesting a substantial disturbance. The overall color is indicative of a mixed stellar population, with evidence of both older, redder stars, particularly in the central region, and younger, bluer stars in the disturbed disk and tidal tail. Dust lanes are subtly apparent within the brighter regions of the disk.
