The galaxy appears as a relatively compact object with an overall elliptical morphology. The light distribution is smooth, suggesting a lack of significant spiral arms or prominent dust lanes. The galaxy's core exhibits a yellowish-orange hue, possibly indicating an older stellar population. The outer regions are dimmer and show hints of bluer colors, which may point to the presence of younger, hotter stars at the outskirts, although this is less pronounced. There is no obvious evidence of ongoing major mergers or significant tidal disturbances, although a subtle asymmetry cannot be ruled out with certainty. Overall, the galaxy presents a mature, relatively quiescent appearance.
