The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. It exhibits a yellow-orange hue, indicating a stellar population dominated by older, evolved stars and a lack of significant ongoing star formation. The morphology appears mostly spheroidal with a high degree of roundness, lacking any prominent spiral arms or a distinct disk structure. There is no visible evidence of recent merger activity or tidal disturbances. The overall structure suggests a mature system.
