The galaxy presents as a relatively compact, luminous object with a predominantly smooth morphology. There is a central bright region, potentially indicative of an active galactic nucleus or a high concentration of stars. The galaxy appears generally round in shape, though with slight irregularities along its outer edges. There are no obvious spiral arm structures or a well-defined disk; its structural organization is indicative of an elliptical galaxy. The color is largely uniform, with a slight shift towards bluer tones near the edge of the galaxy. The mass of the galaxy is substantial, possibly harboring a supermassive black hole at its core. There is no evidence of ongoing major mergers or significant tidal disturbances, but there is a very slight color shift toward the edges that may show hints of star formation.
