The galaxy appears as a moderately bright, elliptical structure. Its light profile is smooth, with no obvious spiral arms or distinct morphological features. There is a slight elongation to its shape, hinting at a possible transition between elliptical and lenticular, but a lack of internal structure makes classification uncertain. The galaxy exhibits a color gradient, with the central region appearing subtly redder compared to the outer regions. There are no apparent signs of recent major mergers or tidal disturbances. The lack of dust lanes and well-defined spiral structure suggest a relatively quiescent star formation history.
