The galaxy presents as a generally smooth, elliptical-like structure. The central region exhibits a high surface brightness, appearing nearly spherical and very concentrated. Surrounding this core, the isophotes become somewhat less round, transitioning to a more intermediate shape, without obvious major axes. There are no discernible spiral arms or a prominent disk component that I can visually confirm.

The galaxy displays a color gradient, with the central bulge appearing slightly yellower-white, indicative of an older stellar population. Moving outward from the center, the galaxy appears to take on a slightly bluer hue, particularly on one side, suggesting regions of more recent star formation.

There is a notable absence of major tidal features or signs of ongoing, large-scale mergers. While some minor irregularity exists in the outer regions, it isn't a textbook example of a dynamically disturbed system. Overall, it presents as a reasonably relaxed system.