The galaxy presents a predominantly smooth, elliptical morphology. The central region exhibits a bright, concentrated core, likely indicative of a significant stellar population density, perhaps hosting a supermassive black hole. There is no obvious dust lane or spiral arm structure visible, suggesting that any disk component is minimal or viewed at a high inclination. The overall color appears somewhat redder than would be expected for a actively star-forming galaxy, which means it is most likely an elliptical galaxy. There are signs of very low star forming activity. The galaxy has a slightly round shape. There is no clear evidence of any major merging events or significant tidal disturbances in the immediate vicinity. It seems to be a settled system without any other apparent galaxies to disturb it.
