The galaxy appears to be elliptical in shape, exhibiting a smooth, centralized light distribution with a high degree of roundness.  The primary color is yellowish, suggesting a stellar population dominated by older, redder stars.  There is a slight hint of asymmetry in the outer regions of the galaxy, potentially indicating past interactions. There is a possible merger occurring, as the image has the indication of tidal tails or minor disturbances. No obvious dust lanes or spiral arm structures are discernible. The galaxy is relatively compact. The overall morphology suggests a system that is well-evolved and possibly quiescent in terms of star formation.
