The galaxy presents as a somewhat elliptical, though not perfectly circular, structure. The primary body of the galaxy exhibits a smooth, centrally concentrated luminosity profile, suggesting an early-type morphology, possibly an elliptical or lenticular galaxy. There is an indication of a secondary, smaller concentration of luminosity extending outwards from the main body. The colors present in the image suggest a mixture of stellar populations, with the central region showing a slight yellowish or orange hue, indicative of older stars. The secondary concentration appears redder in color. Overall, it is not possible to determine if there is a spiral structure, instead, the galaxy appears to have a smooth feature or disk, and the presence of a potential merging event may be indicated.
