The galaxy presents a morphology that appears to be undergoing a possible merger event, or at least exhibiting signs of disturbance within its structure. The primary body shows a centrally concentrated region of high luminosity, surrounded by a more diffuse halo. There is a distinct irregularity in the shape of the galaxy; the isophotes do not exhibit a smooth, elliptical pattern.

The light distribution suggests the presence of multiple components, potentially indicating the remnants of a past or ongoing interaction with another galaxy. There is a slight tail like feature extending from the core. The color gradient appears to be blueish. This likely indicates younger stars in the galaxy, or an ongoing starburst. 
