The galaxy appears as a moderately luminous, centrally concentrated object. Its morphology is generally smooth, with a gradual decrease in surface brightness from the core outwards. The galaxy exhibits a slightly elliptical shape, appearing neither perfectly spherical nor highly elongated. There's a hint of possible disturbance or asymmetry in the outer regions, but it's difficult to discern any distinct spiral arms or other detailed features from this image. The color suggests an older stellar population with a relatively low rate of ongoing star formation, with a higher concentration of stars in the redder bands. There isn't any indication of a major ongoing merger, although there is a hint of a minor disturbance, which may indicate a small interaction event.
