The galaxy presents as an elliptical structure, exhibiting a smooth, largely featureless morphology. It has a near-spherical shape, showing a high degree of central concentration with light gradually decreasing outwards. Color analysis suggests a population of older stars. There is a distinct absence of spiral arms or significant dust lanes. The galaxy appears quiescent, with little to no evidence of ongoing star formation. The galaxy does not appear to be undergoing any major merging activity, although there is some evidence of minor disturbances.
