The galaxy presents as a relatively smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decline in intensity outwards. The galaxy exhibits an orange-yellow hue, suggesting a stellar population dominated by older, redder stars. There is a subtle elongation present, with the galaxy appearing more oval than perfectly circular. No distinct spiral arms or significant dust lanes are visible. There are hints of minor disturbances, though these are subtle. The overall impression is of a quiescent system with little ongoing star formation.
