The galaxy presents an elliptical morphology with a high degree of central concentration. It exhibits a smooth, diffuse light distribution, suggesting an older stellar population with little ongoing star formation. The nucleus is bright and well-defined. The isophotes appear relatively elliptical with a slight flattening. There is some evidence of a faint, extended halo surrounding the main body of the galaxy. The color indices suggest a redder galaxy, indicating a population of older stars, and the absence of prominent blue regions supports low star formation rates. There is a slight disk-like morphology. Evidence of a merger or tidal disturbances appear to be present.
