The galaxy presents as a relatively compact, elliptical-like structure. Its overall form is smooth, with a high degree of central concentration. The core region exhibits a bright, prominent luminosity, suggesting a dense population of stars or potentially an active galactic nucleus, though the current data does not confirm the latter. The galaxy appears slightly flattened, not perfectly spherical, but the flattening is not substantial. The overall color profile suggests a population dominated by older stars, as it is redder in color. There are no prominent spiral arms, bars, or irregular features readily apparent within the galaxy's structure, which further supports its classification as an elliptical galaxy. There are also no clear signs of ongoing major interactions or mergers affecting the galaxy's morphology.
