The galaxy presents an elliptical morphology, appearing relatively smooth in texture. A central, bright region is observed, suggesting a concentration of stars or possible active galactic nucleus activity, however, further spectral data is needed. The overall color profile is a soft blue, indicative of a younger stellar population, possibly undergoing star formation, although it appears to have ended, and the majority of stars are older. The galaxy appears elongated, but is likely still considered to be elliptical, rather than spiral. This galaxy exhibits minor tidal features or distortions, hinting at a prior interaction with another galactic body or the presence of an ongoing, minor disturbance. The galaxy is observed to have a roundness measurement that puts it in-between perfectly round and cigar shaped. There is a moderate probability that this galaxy is a merger.
