The galaxy exhibits a somewhat smooth morphology, with an apparent overall elliptical shape. The central region presents a yellowish hue, indicative of an older stellar population or potentially significant dust obscuration. There are two dominant points of light, which may indicate the presence of a galactic nucleus that is actively merging with another galaxy. The galaxy appears to be relatively compact, suggesting a moderate size. There may be minimal ongoing star formation. Indications of a major merger are present.