The galaxy appears as a smooth, elliptical-like structure, with a concentrated central bulge. There is a gradual fading of light intensity from the center outwards, indicating a diffused stellar population. The galaxy exhibits a yellowish hue, suggesting a population of older stars and a lower rate of on-going star formation. Its overall shape appears elongated, rather than perfectly spherical, hinting at a possible classification between a spherical galaxy and a more elongated elliptical. There's no obvious spiral arm structure or dust lanes visible. A minor disturbance cannot be ruled out.
