The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that transitions into a diffuse halo. The color is primarily yellowish-white, suggesting an older stellar population. There is faint evidence of a disk component but no distinct spiral arm structure is apparent. There may be a very minor disturbance occurring, but no major merging events are visible. Overall, the galaxy appears to be a relatively quiescent system with minimal recent star formation.
