The galaxy appears to be a relatively smooth, elliptical type, with a centrally concentrated bulge. The galaxy exhibits a general lack of distinct features such as spiral arms or significant dust lanes. A slight elongation is observed, deviating from a perfectly circular morphology. A color gradient is also observed, where the core is a yellow hue, becoming more blue towards the edge of the galactic halo. Based on its morphology, the galaxy is likely an older system with a relatively low star formation rate. There is no evidence of any major disturbances or ongoing mergers. The overall light distribution is quite smooth.
