The galaxy appears as a single, somewhat amorphous object with an extended halo. There is a suggestion of a smooth central bulge with an estimated size of approximately 6 kpc. The primary color is a yellowish-white, indicative of an older stellar population.  A region is also visible which is significantly more red-shifted with an intense luminosity. This might be caused by a merger between two galaxies, explaining the unusual morphology. While the system appears mostly undisturbed, closer observation reveals the presence of features indicative of interactions, such as tidal tails or lopsidedness in the overall distribution of light. The overall observed star formation rate appears to be relatively low. The estimated mass of this galaxy indicates it is relatively massive. The primary galactic structure has an overall elliptical shape, with a high likelihood of being a spheroid galaxy. However, one cannot completely rule out other types, based on the potential galactic merger.
