The galaxy appears as a centrally concentrated, generally smooth object. It exhibits a slightly elliptical morphology, appearing mostly rounded. The core is bright, with a gradual falloff in luminosity towards the edges of the galaxy. There is a hint of a disk-like structure, although no defined spiral arms or bar are visible. The galaxy displays a subtle blueish hue indicating some star formation, though the overall color suggests an older stellar population dominates. There is no evidence of any major mergers or strong tidal disturbances affecting the galaxy's structure; however, there may be some minor disturbances present.
