The object presents as a relatively compact galaxy. Its morphology appears largely smooth, exhibiting minimal discernible internal structure. The light distribution is highly concentrated, with a near-circular profile, showing slight deviation toward an intermediate shape rather than elongated. The overall color suggests a population of older stars, although subtle bluer tones are detectable, hinting at ongoing, albeit subdued, star formation. No significant interactions or tidal features with neighboring galaxies are apparent. The galaxy's red shift indicates that it is at a substantial distance.
