The galaxy presents as an elongated, cigar-shaped structure, with a smooth appearance. The central region appears brighter and more condensed than the outer edges, suggesting a higher concentration of stars or luminous material towards the core. The color profile indicates a primarily redder hue in the main body of the galaxy. There is also a prominent region showing blueish emission, possibly indicative of active star formation. There is the potential of a minor disturbance or smaller galaxy merger occurring. 
