The galaxy presents as an elliptical morphology, exhibiting a smooth and largely featureless appearance. The light distribution suggests a spheroidal shape viewed at an angle, appearing elongated or cigar-shaped. The core displays a bright, concentrated luminosity, while the outer regions fade gradually, indicating a lack of distinct spiral arms or prominent disk structures. The color profile indicates an older stellar population with a redder hue, consistent with minimal recent star formation. There is no evident sign of active galactic nuclei activity, tidal disruption or merging. 
