The galaxy presents as a mostly smooth, elliptical morphology, exhibiting a concentrated central bulge that emits a yellow glow indicative of an older stellar population. The light is fairly symmetric, appearing round. There is a hint of a slightly less luminous, extended halo surrounding the main body of the galaxy, fading into the background sky. There does not appear to be any major distortions suggestive of ongoing mergers, though there is a very slight minor disturbance potentially present. No distinct spiral arm structure is visible, and the galaxy appears largely quiescent in terms of current star formation.
