The galaxy presents as a relatively compact, elliptical-like structure. The core region exhibits a high degree of luminosity. The galaxy appears primarily smooth in texture, lacking any prominent spiral arm structures. The morphology suggests a spheroid-dominated system, although the image resolution is limited. There is evidence of some irregularity in the outer isophotes, possibly indicating a past or ongoing minor interaction or merger event, or internal dust features. There are signs of a dimmer, smaller galaxy that appears to be interacting with it, or is a background galaxy. The color index indicates a moderate population of older stars, but there is evidence of some blue light. The galaxy is not perfectly spherical, but instead slightly flattened.
