The galaxy appears as a concentrated, centrally bright, and relatively smooth elliptical-like structure. The light distribution suggests a high degree of central concentration, with a smooth falloff in intensity towards the outer regions, lacking well-defined spiral arms or prominent features like dust lanes or distinct star-forming regions.

The galaxy's color exhibits a yellow-red hue, which would typically indicate an older stellar population. The overall smoothness and color suggest this galaxy is most likely an elliptical galaxy, with a small chance of being a lenticular galaxy seen face-on. There is no evidence of any major disturbances or ongoing mergers. 
