The galaxy presents as a moderately bright, elliptical-like object with a relatively smooth, amorphous structure. The central region exhibits a higher concentration of light, gradually decreasing outwards. The overall color appears somewhat redder than the surrounding field objects, indicating a potentially older stellar population. There are no readily apparent spiral arms or dust lanes visible. The morphology is largely undisturbed, showing no major signs of interaction or recent merger events. The galaxy exhibits an intermediate roundness.
