The galaxy appears as a concentrated, somewhat elliptical structure with a smooth overall morphology. There is a slight elongation, deviating from a perfectly circular shape. The primary color is a yellow/orange hue, suggesting a population of older stars and potentially significant dust content. There is an absence of well-defined spiral arms or distinct features typically associated with ongoing, high-intensity star formation. Based on the fuzzy edges, the galaxy appears to be at a considerable distance. There is some evidence of minor disturbances in the galaxy's shape, possibly indicative of a past or ongoing interaction with another galaxy. There are some indications of potentially merging components.
