The galaxy presents a smooth, largely featureless morphology. It appears nearly round, with a slight deviation towards a more elliptical shape. The light distribution is concentrated towards the center, suggesting a bulge-dominated structure. There are no visible spiral arms or significant dust lanes. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a slightly bluer outer region. This color variation may indicate a difference in stellar populations, with older stars concentrated in the core and younger stars in the outer parts. No signs of major ongoing mergers or tidal disturbances are apparent, though the possibility of minor interactions cannot be excluded based on the image alone.
