The galaxy presents as a smooth, elliptical form. The overall color profile appears relatively uniform, trending towards a yellow-red hue in the central bulge. There are no distinct spiral arms or significant dust lanes visible, suggesting a lack of ongoing, large-scale star formation. The galaxy's shape shows deviation from perfect sphericity, appearing somewhat elongated. There is no obvious evidence of active galactic nuclei activity or any ongoing major merger events, although subtle distortions might indicate minor gravitational interactions. The galaxy exhibits a degree of central concentration, with light intensity decreasing gradually from the core to the outer edges. Overall, the morphological characteristics suggest a galaxy that has largely exhausted its gas reserves, is dominated by an older stellar population, and is likely undergoing passive evolution.
