The galaxy appears as a slightly elongated, smooth structure with a relatively concentrated central region. There is no immediately visible spiral arm structure or significant dust lane obscuration. The light profile suggests a possible elliptical morphology. The galaxy exhibits a bluish hue, which may indicate the presence of some younger stellar populations and ongoing, though possibly minimal, star formation. The lack of prominent features suggests that the system is relatively undisturbed, potentially evolving in isolation without recent major mergers. There might be some minor tidal disturbance. Further observations are needed to confirm its exact morphology and star formation history.
