The galaxy presents as a single, concentrated light source. Its morphology appears largely smooth and elliptical, with a high degree of central concentration. There is no evidence of spiral arm structures or a prominent disk component based on visual inspection. The color profile is relatively uniform, exhibiting a yellow/red hue throughout the galaxy, suggesting an older stellar population and reduced ongoing star formation. The object appears quite round and there is no visual indication of any ongoing merging activity or tidal disturbances. It is a relatively compact system.
