The galaxy presents with a disturbed morphology, exhibiting characteristics suggestive of an ongoing or recent merger event. The primary body of the galaxy appears diffuse, lacking a well-defined spiral arm structure or a prominent bulge. There are indications of tidal tails or extended debris fields, primarily blue in color, emanating from the main galactic body, further supporting the classification as a merging system. Some areas show an increased concentration of blue light, which implies active star formation within these disturbed regions, although the overall rate of star formation is relatively low. The system appears to have multiple components undergoing gravitational interaction, contributing to the observed irregular shape and the dispersion of galactic material. The galaxy is not particularly luminous, with the primary body appearing moderately faint.
