The galaxy presents as a relatively smooth, elliptical structure. It exhibits a central concentration of light, with the intensity gradually decreasing outwards. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the galaxy's core. There is little evidence of distinct spiral arms or significant dust lanes, implying a lack of ongoing, large-scale star formation. The galaxy appears moderately rounded, tending towards an elliptical shape, with a slight elongation visible along one axis. No major merger events or tidal disturbances are immediately apparent, though subtle irregularities might suggest minor interactions in its past. Overall, the galaxy presents as a fairly evolved system.
