The galaxy presents as an elliptical morphology, appearing largely smooth and lacking prominent spiral arm structures or a central bar. Its shape is roughly rounded, exhibiting only a slight elongation. A central bulge is evident, appearing bright and concentrated. The color gradient suggests an older stellar population, transitioning from a yellowish-orange core to a slightly bluer halo. There is no obvious active galactic nucleus or distinct dust lane visible. No signs of major mergers or significant tidal disturbances are discernible. The overall light distribution is consistent with a relatively evolved, quiescent galaxy.
