The galaxy presents as a largely elliptical structure, with a smooth, diffuse light distribution and a high degree of central concentration. It has a noticeable yellowish hue, hinting at a relatively older stellar population. There is a lack of discernible spiral arms or distinct dust lanes. The general roundness of the galaxy indicates a minimal level of rotational support, suggestive of a galaxy dominated by random stellar motions. There is a slight asymmetry in the light distribution, potentially suggesting an ongoing or recent minor interaction with a smaller companion. While appearing mostly undisturbed, there is a faint hint of possible tidal features in the immediate vicinity.
