The galaxy presents as a centrally concentrated elliptical or S0 type. It exhibits a smooth, spheroidal morphology with no apparent spiral arm structure or prominent dust lanes visible. The galaxy's color profile suggests an older stellar population, with a yellow to reddish hue dominating its overall appearance. The light is relatively evenly distributed, decreasing smoothly from the core outwards. There is little to no evidence of ongoing major star formation activity based on the lack of bluer, irregular regions. The galaxy shows minimal signs of interaction or disturbance, appearing largely isolated and undisturbed.
