The galaxy presents as a centrally concentrated system. The light profile exhibits a smooth appearance, with a high degree of central concentration indicative of an elliptical galaxy. It is nearly circular in appearance, with a slight elongation along a position angle approximately northwest to southeast. The central region displays a bright, relatively uniform color, likely due to an older stellar population dominating the light output. There is no clear evidence of spiral arm structures or a distinct galactic disk. The overall color suggests a relatively low level of on-going star formation, which is congruent with it's smooth profile. There are no apparent signs of tidal disturbances or merging events within the immediate vicinity of the galaxy, suggesting a relatively undisturbed evolutionary history.
