The galaxy presents as a relatively compact object, exhibiting a smooth and largely featureless morphology. Its overall shape approximates a circular form, appearing quite rounded. The light profile shows a central concentration, diminishing gradually towards the outer regions. Coloration is generally yellowish, suggesting a dominant population of older stars. No obvious spiral arms, bars, or significant dust lanes are discernible. There is no obvious signs of a major merger in progress, or strong tidal disturbances. Evidence suggests it is an evolved system with minimal ongoing star formation.
