The galaxy presents as a predominantly smooth object, exhibiting an elliptical morphology with no apparent spiral arm structures or significant disk features. The central region appears intensely luminous, suggesting a high concentration of stars or potentially an active galactic nucleus (AGN), although this cannot be definitively confirmed from the image alone. The color gradient across the galaxy seems relatively uniform, trending towards redder hues. This color profile could indicate an older stellar population with lower rates of ongoing star formation throughout the galaxy. There is no obvious sign of any recent merger events or tidal disturbances, and the galaxy appears relatively undisturbed.
