The galaxy presents as a relatively smooth, elongated structure. Its overall shape is somewhat cigar-shaped, lacking a well-defined spiral arm structure. There appears to be a brighter, more concentrated central bulge. The galaxy exhibits a blueish hue, particularly in the central regions. Fainter, diffuse extensions emanate from the central body, suggesting possible tidal features or ongoing interactions. Based on these observations, this galaxy exhibits potential signs of disturbance, possibly due to a past or ongoing merger event. Star formation appears to be moderate within the galactic body.
