The galaxy exhibits an overall elliptical morphology, with a slight elongation along its major axis. The central region displays a smooth, concentrated bulge. The color profile indicates a mixture of stellar populations. The core is a yellow-orange hue, suggesting the presence of older, redder stars, whereas there are distinct blue regions within the galaxy, which could be pockets of star formation within the galaxy. Some evidence for tidal tails extending out from the central galaxy structure suggests that it is a product of one or more past galaxy mergers or significant interactions, making it a potential candidate for ongoing or recent merger activity. 
