The galaxy presents as a relatively compact structure with a concentrated central region. Its overall color suggests a mix of stellar populations, with a dominant yellowish hue indicating a significant population of older stars. The morphology leans toward being smooth and elliptical, with a high degree of central concentration. There is a slight suggestion of disk-like characteristics and some irregularities in the outer regions, possibly hinting at past or ongoing interactions. There does not appear to be a great deal of recent star formation activity taking place. The galaxy appears to be somewhat massive.
