The galaxy presents a primarily smooth morphology, appearing largely spheroidal in shape. There is evidence of an interaction or merger, where the central region of the galaxy appears disturbed. A secondary, smaller concentration of light appears separated from the main body, possibly the remnant core of another galaxy. The galaxy exhibits a yellow hue, suggesting a population of older stars and relatively low star formation activity. There is not an obvious disk structure. The galaxy appears to be at intermediate distance.
