The galaxy presents a notably smooth morphology with a largely elliptical shape, though some minor irregularities suggest potential disturbances. The light distribution indicates a concentrated central bulge, surrounded by a more diffuse halo. Color gradients are subtle; the core exhibits a slightly yellow hue, transitioning to redder tones in the outer regions, possibly indicating older stellar populations toward the periphery. Two distinct bright concentrations are observed. These are likely core areas that are in the process of merging, as they are connected by a small amount of light. Overall, there is evidence of moderate levels of ongoing star formation. The galaxy is of considerable mass, with a significant contribution from both stellar and dark matter components.
