The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Progressing outward from the core, the galaxy fades into a more diffuse halo. 

A notable feature is the apparent minor disturbance or potential tidal tail extending from the left side of the galaxy. This structure exhibits a reddish color, potentially indicating either a region of ongoing star formation or dust obscuration. It is possible this feature is a result of a past minor merger event.

The overall morphology suggests a galaxy that has largely completed its major merging history, with a significant fraction of its stellar population being relatively old. However, the aforementioned tidal tail suggests the possibility of recent or ongoing interaction.
