The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of central concentration. The core region is luminous with a yellowish hue, suggesting an older stellar population. A slight extension of the isophotes is apparent, giving it a somewhat elongated shape. The outer regions display a fainter, less distinct profile with a subtle blue tint in the disk, indicative of some ongoing star formation. No prominent spiral arm structures or dust lanes are clearly visible, though there may be minor disturbances, but it appears largely undisturbed. The overall color suggests a relatively evolved system, with a significant fraction of older stars but still retaining some star-forming regions.
