The galaxy appears as an elliptical or lenticular system, characterized by a smooth, concentrated central bulge of yellow light. Its overall shape is moderately elliptical, appearing more elongated than perfectly circular. There may be a faint, diffuse disk surrounding the central bulge, exhibiting a subtle blue tint indicating the presence of some younger stellar populations. However, it appears primarily composed of older stars. There are no signs of significant ongoing star formation. The galaxy appears relatively isolated, with no clear evidence of major tidal disturbances or ongoing mergers, though a potential slight disturbance cannot be ruled out.
