This galaxy presents as a somewhat elongated, centrally concentrated object. A dominant, smooth bulge is apparent, exhibiting a high degree of spheroidal symmetry. The light distribution fades gradually from the bright nucleus outwards, with a noticeable absence of defined spiral arms or prominent disk features. Faint extensions or tidal features, or perhaps an artifact, can be observed near the top of the galaxy, but they are not as distinct. There are very subtle color gradients within the galaxy, with bluer tones near the center and possibly slightly redder hues in the outer regions. There are also slight disturbances within the main body of the galaxy, but not on a major scale. Overall, the galaxy appears to be a relatively evolved system, showing properties that might be observed in a galaxy that has undergone significant dynamical relaxation.
