The galaxy presents as a relatively compact object with an apparent elongation along one axis, suggesting a possible disk-like structure viewed at an angle. The central region exhibits a bright, concentrated core. A fainter extension of light is observed to emanate from the core region to one side, indicative of a potential tidal tail or arm-like structure. The colour profile varies across the galaxy, with the core appearing bluer, possibly indicating a higher concentration of younger, hotter stars, while the outer regions appear redder in comparison, potentially due to an older stellar population or dust obscuration. There appears to be a minor disturbance occurring with the merging of a smaller galaxy. 
