The galaxy presents as a slightly elongated spheroid with a smooth, diffuse appearance. Its color profile suggests a mixture of stellar populations, with a central region exhibiting a warmer, possibly redder hue, grading into cooler blue tones towards the outer edges. There is no distinct nucleus or spiral arm structure readily apparent. The general morphology points toward an elliptical or lenticular classification, lacking significant recent star formation. Faint disturbances are visible, hinting at possible minor gravitational interactions or past merger events, although the overall structure is not highly disrupted. 
