The galaxy presents a generally smooth morphology, exhibiting a somewhat elongated, elliptical shape. The core region displays a bright, concentrated luminosity, suggestive of a substantial stellar density. Moving outward from the core, the light intensity gradually diminishes, with no prominent spiral arm structures or distinct features readily apparent. There is a subtle color gradient observed; the central region appears to be slightly more yellowish-white, potentially indicative of older stellar populations, while the outer regions show a faint bluish tinge, hinting at more recent, albeit low-level, star formation activity. No evidence of major mergers or significant tidal disturbances are visible. Overall, the galaxy appears to be a relatively quiescent system.
