The galaxy exhibits a generally smooth morphology, with a central, bright bulge exhibiting a relatively round shape. There is a hint of a disk component but it appears indistinct, contributing less to the overall light profile. The overall appearance is undisturbed, showing no strong signs of recent major merging events.

The light from the galaxy is skewed slightly towards the redder part of the spectrum, suggesting an older stellar population may dominate the light being observed. Given the apparent smoothness and the redder color, this galaxy is likely an early-type galaxy.
