The galaxy presents as a luminous object with a largely smooth morphology. The central region exhibits a high concentration of light, indicative of a prominent galactic nucleus or bulge. The light falls off gradually in a roughly elliptical shape moving away from the central bulge. Some subtle irregularities are present, suggesting a potential for minor tidal disturbances or internal structures. The overall color appears relatively uniform, trending towards a slightly redder hue. The light distribution suggests that the galaxy is likely an elliptical, or possibly a lenticular galaxy viewed with a slight inclination.
