The galaxy presents as a centrally concentrated object with a smooth, diffuse light distribution. It exhibits an elliptical morphology, with an axis ratio that is close to circular but subtly elongated. The core of the galaxy appears bright and yellow, indicative of an older stellar population dominated by redder stars, possibly with a substantial population of intermediate age stars as well. The outer regions display a fainter, more blue-green hue, suggesting a small contribution from younger, hotter stars and a low level of ongoing star formation, with a total mass estimated to be over 10^10 solar masses. There are no obvious signs of spiral arms, a central bar, or significant dust lanes. The lack of any strong distortions suggests the system is relatively relaxed, with no major ongoing or recent merger events.
