The galaxy presents a generally smooth, elliptical morphology. It appears nearly spherical, with a high degree of central concentration of light. The central region exhibits a bright, yellowish-white glow, suggesting a population of older stars. There is a faint, diffuse halo extending outwards from the central region, which appears slightly bluer than the core, indicating the possible presence of a younger stellar population or ongoing star formation, albeit at a relatively low rate. No distinct spiral arms or a prominent disk structure are apparent. There is no evidence of any significant mergers or tidal disturbances. The overall impression is that of a well-formed, evolved galaxy.
