The galaxy appears as a moderately bright, somewhat compact object. Its overall morphology appears to be relatively smooth, with a high degree of central concentration. The shape is neither perfectly spherical nor highly elongated, suggesting an elliptical or possibly a lenticular classification. There is some evidence of a possible minor interaction or disturbance in the structure, given the slight asymmetry in its morphology. 

The galaxy exhibits a yellowish hue, indicating the presence of an older stellar population. It is likely a massive galaxy with moderate ongoing star formation, which causes it to appear so bright. This object could potentially be the result of an ongoing merger.
