The galaxy presents a generally smooth and elliptical morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. The outer regions fade gradually without any distinct spiral arm features. The overall shape is somewhat elongated, potentially indicating a deviation from a perfectly spherical structure. The galaxy exhibits a relatively blue hue, particularly concentrated toward the center, suggesting the presence of some younger stars, however the smooth morphology is consistent with a low star formation rate. No signs of a major merger event are obvious in the image, although a subtle asymmetry suggests a potential minor interaction.
