This galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated morphology. The central region exhibits a yellowish hue, indicative of an older stellar population. Surrounding this core is a diffuse, bluer envelope suggesting the presence of younger stars, possibly in a disk-like structure. There is no clear evidence of spiral arm structure or a prominent bar. While the overall appearance is relatively undisturbed, there may be some minor asymmetries or irregularities in the outer regions, potentially hinting at past or ongoing interactions. The galaxy appears to be in a relatively quiescent state of star formation.
