The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution is concentrated toward the center, with a gradual decrease in intensity outward. The color appears predominantly yellow-red, suggesting an older stellar population and a lower rate of recent star formation. The shape appears moderately elliptical, not perfectly spherical, but also not highly elongated. There is no clear evidence of spiral arms, a bar structure, or significant dust lanes. No signs of a major ongoing merger are visible, though there might be subtle signs of minor disturbances within the galaxy's morphology.
