The galaxy presents as a central, moderately bright, elliptical form. A concentrated nucleus transitions into a smoothly diffused stellar distribution, without prominent spiral arm structures. Its overall color profile suggests an older stellar population, consistent with a quiescent or post-starburst phase. The morphology is dominated by a bulge, exhibiting a somewhat rounded shape. Indications of minor tidal disturbances or interactions are present, but are subtle. No ongoing major merger events are apparent. The galaxy appears relatively isolated.
