The galaxy presents as a luminous elliptical structure, exhibiting a concentrated central bulge that gradually diffuses outward into a less distinct halo. The color gradient shifts from a yellowish-white core towards a redder periphery, indicative of an older stellar population dominating the outer regions. There appears to be little to no evidence of spiral arm structure or active star formation as observed in the image. The overall morphology suggests a relatively smooth, evolved system, possibly with a low star formation rate. The shape is more akin to a flattened sphere. Some subtle hints of disturbances in the outer halo may indicate past minor merger events. 
