The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing as a bright, roughly circular core with a yellowish hue. The galaxy's overall shape is quite round, with only a slight deviation from perfect circularity. There is a lack of any obvious spiral arm structures or other distinct features typically associated with disk galaxies. The outer regions of the galaxy gradually fade into the background, indicating a relatively smooth decline in stellar density. There is no obvious evidence of any major ongoing merging events or significant disturbances in the galaxy's overall structure, although subtle irregularities may be present at a small scale. The color suggests an older stellar population with relatively low ongoing star formation. 
