The galaxy presents a relatively smooth morphology, with a dominant, round central bulge exhibiting a yellowish-orange hue. A smaller, less distinct component is visible, possibly indicating a minor disturbance or interaction. The object appears compact, suggesting a potentially spheroidal or elliptical classification, rather than a spiral. The overall color indicates a population of older stars and a relatively low rate of ongoing star formation. There are no prominent spiral arms or dust lanes visible in the image, which further supports a classification leaning towards an elliptical or lenticular galaxy type. The system appears to be experiencing a potential merging event.
