The galaxy appears as a centrally concentrated object with a smooth overall morphology. A bright, yellowish core gradually fades into a diffuse, bluish halo. The galaxy exhibits an elliptical or lenticular shape, with no obvious spiral arm structures. The smooth light distribution suggests a relatively old stellar population with minimal ongoing star formation. There might be some minor tidal disturbances hinting at past or ongoing interactions, but not significant enough to classify the galaxy as a major merger. Overall, it appears to be a fairly evolved system.