The galaxy exhibits a complex morphology, suggestive of an interacting system or recent merger event. The primary structure appears to be a relatively smooth, centrally concentrated component with an extended halo. A distinct, elongated feature emanates from this central region, showing a knot of intense star formation towards the end. The overall color profile indicates a mix of stellar populations, with the central region displaying a yellowish hue, and hints of bluer regions possibly indicating younger stars. There is a disturbance in the galaxy's structure. The galaxy exhibits moderate star formation activity, evidenced by the knot along the tidal tail structure. The estimated size of the galaxy is approximately 8 kpc.
