This galaxy presents as a somewhat irregular structure with a moderately bright core region. The overall morphology appears disk-like, though the disk is significantly disturbed. There is a possible arm structure emanating from the central region, however, this is disrupted with clear signs of tidal features.

The color profile suggests ongoing star formation within the disk, indicated by the bluer hues in the spiral arm features. The central bulge, appears slightly redder, potentially indicative of an older stellar population. Based on the disturbed morphology, it is likely this galaxy has experienced, or is experiencing, a merger event with another galaxy. The outskirts of this galaxy are rather faint.
