The galaxy presents a predominantly smooth, elliptical morphology. The light is concentrated towards a bright, almost stellar-like, core suggesting the presence of an active galactic nucleus or a dense stellar population in the galactic center. A diffuse, flattened halo surrounds the core, exhibiting a bluish tint. The disk exhibits no distinct spiral arm structure. There is a slight asymmetry visible in the halo, possibly indicating minor gravitational disturbance or a past minor merger event. Overall, the galaxy appears to be relatively undisturbed and lacks strong evidence of ongoing major star formation.
