The galaxy presents as a concentrated central bulge with some surrounding diffuse material. It shows a yellowish-orange hue, suggesting a population of older stars and a relatively low rate of on-going star formation. The object appears somewhat disturbed, with an irregular shape that hints at a possible interaction or merger event. This morphology is seen with a combination of features: Some disturbance is present but most likely a merging event is occurring. The size of the galaxy is appreciable, indicating a substantial mass. The presence of the older stellar population suggests a galaxy at a relatively late stage of its evolution. 
