The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its morphology is characterized by a concentrated central bulge that diminishes into a halo with no apparent spiral arm structure. The core presents a strong orange hue, indicating a higher concentration of older stars or dust obscuration. The overall shape of the galaxy is generally round, with no obvious elongations or distortions. The galaxy shows no signs of major disturbances such as tidal tails or multiple nuclei, suggesting it has not undergone a recent major merger event. There are some slight irregularities in the outer halo of the galaxy, showing minimal evidence of a minor disturbance or interaction.
