The galaxy presents as a relatively smooth, elliptical morphology, with no obvious spiral arm structures or distinct disk features visible. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue. This color suggests a population of older stars, indicating a potentially quiescent star formation rate within the bulge region. The overall shape is somewhat elongated, but not significantly so; it appears largely spheroidal. There are subtle hints of extended diffuse light surrounding the central region, possibly indicating a halo of older stars or tidally stripped material. No major or minor disturbances indicative of ongoing or recent merger activity are readily apparent in the galaxy's structure.
