The galaxy presents a generally smooth, elliptical morphology. There is a central concentration of light that appears yellowish-white, indicating an older stellar population likely dominating the core. This central region blends gradually into a less intensely luminous, more diffuse halo. A slight bluing is observed in the outer regions of the galaxy, suggesting the presence of some younger, hotter stars, though this is less prominent than the core. There is no visible evidence of spiral arms or a distinct disk structure. No major morphological disturbances are noted in this image, it appears to be a relatively isolated galaxy.
