The galaxy presents as a smooth, elliptical-like structure with a concentrated, bright core. The light distribution is relatively even, with a gradual decrease in intensity moving outward from the central region. The object exhibits a warm, yellowish hue, suggesting an older stellar population. There is no evidence of spiral arms, dust lanes, or significant star-forming regions discernible in this image. The overall form is more rounded than highly elongated. There appears to be no major interactions with other galaxies and only a minor chance of disturbance. It can be described as a large galaxy that does not form many stars.
