The galaxy presents as a relatively smooth, elliptical morphology. The primary component of the galaxy exhibits a yellow-white hue, indicative of an older stellar population. The central region appears more concentrated in brightness and is more yellow, suggesting a greater density of older, cooler stars and minimal dust obscuration. There is a suggestion of a faint, diffuse halo surrounding the main body, which is more apparent on the left side of the galaxy. The halo exhibits a slightly bluer tinge compared to the core, possibly indicating a younger stellar population. There appears to be a satellite galaxy that is close in proximity to the central mass. This satellite galaxy has a more orange-yellow hue.
