The galaxy presents a largely smooth morphology, appearing as a diffuse, centrally concentrated object. Its overall shape approximates a flattened spheroid, but with no readily discernible spiral arm structures or bar features. The radial color profile exhibits a noticeable trend, transitioning from a more yellow/orange hue at its core to a slightly bluer color in the outer regions. This suggests a possible variation in stellar populations or dust content. No significant signs of ongoing major mergers or strong tidal disturbances are observed in the immediate vicinity of the galaxy.
