The galaxy presents an elliptical morphology, with a smooth, diffuse appearance indicative of an older stellar population. The central bulge appears as a bright, concentrated region of yellowish light. The outer regions of the galaxy gradually fade into the background, exhibiting a less concentrated distribution of stars. There is a subtle hint of distortion or disturbance in the galaxy's overall shape, but its symmetry is relatively intact. There is no apparent dust lane or prominent spiral arm structure visible. The observed color suggests a low rate of on-going star formation within the galaxy.
