The galaxy appears to be a relatively bright, moderately sized object with a smooth, elliptical morphology. Its core exhibits a concentrated luminosity profile, suggesting a dense stellar population. The overall color appears to be slightly redder, hinting at an older stellar population with a lower rate of current star formation. There is a subtle asymmetry present, possibly indicating a minor gravitational interaction or internal disturbance. The galaxy is neither perfectly spherical nor highly elongated, with an intermediate degree of roundness. Faint wisps of light extend outwards, but there are no prominent spiral arms or strong indications of a major ongoing merger event.
