The galaxy presents as a concentrated, elliptical structure. Its central region is a bright, yellowish-white, indicating a high density of older stars. Moving outward from the center, the color shifts to a slightly bluer hue. The galaxy appears relatively smooth and uniform with no obvious spiral arm structures or dust lanes discernible in this image. The light distribution suggests a gradual decline in stellar density from the core to the outer regions, with no clear signs of active star formation in the outskirts. The galaxy's overall shape is generally elliptical with a moderate ellipticity. No indications of tidal tails, asymmetries, or other signs of recent major merger activity are observed.
