The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a largely featureless morphology. It presents with a centrally concentrated bulge, brighter and more yellow in color, suggesting an older stellar population in that region. The outer regions of the galaxy fade in intensity and exhibit a bluer hue, potentially indicating more recent, albeit subdued, star formation. The overall shape is somewhat elongated, displaying an intermediate ellipticity that deviates from perfectly spherical. There is a subtle hint of possible minor gravitational disturbance on one side, suggesting a prior interaction or merging event, though this is not definitively clear from the available imagery. The color gradients indicate a progression from older stars in the center to a younger population at the edges. The galaxy's overall structure suggests a system undergoing a slow rate of star formation.
