The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a concentrated, bright yellowish core, indicative of an older stellar population and potentially a supermassive black hole actively accreting material. There is a suggestion of some minor disturbances to the galaxy's overall structure. The light is redshifted, and the inferred size suggests a significant stellar mass and star formation rate. There are potential signs of recent or ongoing merger activity. Overall the galaxy appears to be in an active phase of evolution.
