The galaxy presents a predominantly smooth, elliptical morphology. The light distribution appears relatively even across the galaxy's body, with a concentrated central region of higher luminosity, likely indicating a prominent galactic nucleus. The galaxy appears somewhat flattened, with a major axis extending horizontally in the image. A hint of a faint, extended disk-like structure may be present along this axis, but it is not clearly defined. There is no strong evidence of spiral arm structure or prominent dust lanes within the galaxy. The color profile indicates a population of older stars. There are also no indications of major disturbances or ongoing mergers in the surrounding environment.
