The galaxy appears as a relatively smooth, elliptical structure. Its central region exhibits a high surface brightness, suggesting a concentrated stellar population. The light gradually diminishes towards the outer regions, which are less defined. The galaxy's overall shape is moderately elongated, exhibiting an axis ratio that deviates from perfect circularity. It is not perfectly round, and it also is not very elongated. Faint, diffuse structures can be perceived within the galaxy's outer edges. There are no prominent spiral arms. The galaxy displays a bluer hue on the left side with yellower colors in the center, suggesting some star formation activity.
