This galaxy presents as an elliptical or lenticular system, exhibiting a generally smooth morphology without prominent spiral arm structures. The light distribution appears relatively uniform, suggesting an older stellar population and reduced ongoing star formation activity. The object displays a radial color gradient, with the central region exhibiting a yellow hue that transitions to redder tones towards the outer edges. The symmetrical light profile indicates a relaxed state, with no obvious signs of recent major merger events or significant tidal disturbances. The lack of substantial dust lanes or prominent features suggest a relatively quiescent system with a well-mixed stellar population.
