The galaxy presents as a relatively compact, luminous object. The overall morphology is suggestive of an elliptical galaxy, although some features indicate a possible merger event or tidal disturbance.

The central region appears very bright, with what seems to be two high concentration areas, possibly indicating dual galactic cores. The shape of the galaxy appears irregular, with no prominent spiral arm structure detected.

The color distribution is dominated by redder wavelengths, implying a stellar population comprised primarily of older stars with suppressed star formation. However, given the bright magnitudes in the g,r and z bands, some ongoing star formation is not completely ruled out, but is likely to be low. It appears to be a very massive galaxy.

Evidence of minor asymmetries or distortions in the outer regions of the galaxy exist, possibly due to interaction with another galaxy. A more detailed analysis of the galaxy’s velocity field would be beneficial in confirming this merger status.
