The galaxy presents as a moderately luminous object with an overall elliptical morphology. It exhibits a smooth, relatively featureless appearance, suggesting a lack of prominent spiral arms or significant dust lanes. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards from the core. Its color appears slightly yellow, possibly indicating an older stellar population with a lower rate of star formation. There is a slight asymmetry to the galaxy’s shape, with a possible minor disturbance observable. The galaxy does not appear to be undergoing a major merging event. The observed characteristics are consistent with a galaxy of substantial mass, possibly around the mass of our milky way.
