The galaxy presents an overall smooth, elliptical morphology. The central region exhibits a concentrated, bright core, suggestive of a substantial bulge component. The light distribution transitions from a reddish hue in the core to a more greenish-yellow tinge in the outer regions. There is a slight elongation to the galaxy's shape, deviating from perfect circularity. While the overall structure appears largely undisturbed, there's a hint of asymmetry or minor structural irregularity in the outer regions, possibly indicating a past minor interaction or ongoing accretion. Star formation is present, but not dominant, with the green color indicating the presence of younger stars.
