The galaxy presents as a relatively smooth, elliptical morphology. Its central region exhibits a high concentration of light, appearing bright and somewhat yellowish, suggestive of an older stellar population. Moving outward from the core, the light gradually decreases in intensity. The outer regions show subtle hints of a disk-like structure. Overall, there is no obvious evidence of spiral arms or a strong bar feature. The galaxy appears fairly isolated, showing no significant signs of a major merger event. There is a slight hint of minor tidal disturbance.
