This galaxy presents as a disrupted, elongated structure with a faint, diffuse outer halo. The main body appears as a curved arm, with the southwestern portion appearing more tightly wound than the northeastern portion. A distinct knot of bluer light, potentially a region of active star formation, is observed at the terminus of the northeastern section of the arm. The core region of the galaxy exhibits a smoother, yellower profile, indicative of an older stellar population. The overall shape and the presence of a bright knot suggest a possible recent interaction or merger event.
