The galaxy presents as a centralized, moderately bright object with an elliptical morphology. The light distribution appears relatively smooth and diffuse. I observe a slight yellow tinge to its color, indicating an older stellar population. The overall structure lacks prominent spiral arms or distinct features typically associated with actively star-forming galaxies. There is minimal evidence of tidal disturbances or ongoing merger activity based on the morphology. The light distribution suggests a spheroidal structure rather than a disk-dominated system.
