This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. The light is concentrated towards the center, with a bright, prominent nucleus that suggests a high density of stars in the core. The color gradient transitions from a yellowish-white core to a reddish halo, indicative of an aging stellar population. The galaxy shows no apparent spiral arm structure or significant dust lanes. There are no indications of major disturbances due to merging activity, although a possible faint irregularity could suggest a minor interaction in the past.
