The galaxy presents a largely smooth morphology, appearing as a single, relatively undisturbed object. The shape approximates a slightly elongated ellipse, exhibiting a moderate degree of roundness. The color profile indicates a central concentration of light, likely corresponding to an older stellar population exhibiting a redder hue. This gradually transitions to a bluer, less concentrated halo surrounding the central region. Subtle variations in color and light intensity throughout the galaxy's structure suggest possible variations in stellar density and age. There are no obvious signs of major mergers or significant tidal disturbances impacting its overall structure. Star formation is apparent, although not dominating the galaxy.
