The galaxy presents a primarily smooth morphology, with a high probability of being an elliptical. Its apparent size is small, but given its estimated redshift, implying a considerable distance, its intrinsic size is likely substantial, perhaps in the range of several kiloparsecs. The galaxy exhibits a colour gradient, appearing more luminous and yellowish in the central region, suggesting a population of older, evolved stars. A distinct redder clump is observed, possibly indicating an area of intense star formation activity, dust obscuration, or a smaller merging companion. The overall structure shows some possible tidal disturbances, indicative of past or ongoing interactions, however the galaxy appears to be quite relaxed overall.
