The galaxy presents as an elongated structure, exhibiting a primary axis of higher luminosity and a fainter extension along the perpendicular axis. The overall light distribution suggests a central bulge region with a gradual decrease in surface brightness towards the edges. There is evidence of morphological disturbance, potentially caused by a minor gravitational interaction with another object. This interaction is suggested by an irregular structure on one side of the galaxy that appears as a separate entity, though it is difficult to assess whether it is a satellite galaxy or merely an asymmetrical feature within the main galaxy. The observed color gradient might indicate varying stellar populations throughout the galactic body, with a potential for differing rates of star formation depending on the region. The presence of a substantial disk component appears to be a possibility.
