The galaxy presents as a single, largely featureless object. Its morphology appears elliptical, with a high degree of central concentration. The light profile suggests a smooth and diffuse distribution of stellar populations, lacking the defined spiral arms or bar structures characteristic of disk galaxies. Color gradients are subtle, with a central region exhibiting a yellower hue, possibly indicative of older stellar populations or dust obscuration. The outer regions appear slightly bluer, which might represent younger stars. Overall, the galaxy exhibits no evidence of significant ongoing star formation, mergers, or tidal disturbances.
