The galaxy presents as a single, concentrated object with a centrally-peaked light profile, appearing generally smooth in texture. Its overall shape is ellipsoidal, tending towards round. A subtle color gradient is discernible, transitioning from a yellowish-white core to a bluish halo. There is no obvious spiral arm structure or dust lane features visible. The galaxy does not show any strong signs of ongoing merger activity or major disturbance in its morphology, although some minor asymmetry or disturbance cannot be ruled out given image resolution. The overall light distribution suggests that the galaxy has a relatively old stellar population, concentrated in the bulge, with a lower level of star formation extending outwards.
