The galaxy presents as a smooth, elliptical-like structure, elongated in shape. A concentration of light is visible towards the galactic center, appearing a yellowish hue. The galaxy appears largely homogenous in color and texture. Some subtle blueish tones are observed toward the outer regions. The lack of defined spiral arms or significant dust lanes suggests an older stellar population or a galaxy that has undergone significant morphological transformation. There is no obvious visual evidence of a major merger event in the recent past, though subtle irregularities could indicate minor disturbances.
