The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is a bright, relatively compact core region that fades gradually outward into a more diffuse halo. The overall shape appears approximately elliptical, displaying a slight deviation from perfect circularity. Hints of bluer hues are visible within the central region, potentially indicating the presence of younger stellar populations or ongoing star formation, although this is not overtly pronounced. Faint, subtle irregularities are visible in the outer regions, which may point to minor interactions or disturbances in its gravitational history. No prominent spiral arm structures or a well-defined disk are discernible within the image resolution.
