The galaxy presents a somewhat elongated, cigar-shaped morphology. The central region exhibits a high degree of luminosity, with a primarily yellow hue. The color suggests a substantial population of older stars. There is a subtle disk-like structure present but it appears largely featureless; likely due to its distance. The outer edges display a hint of bluer light. This indicates recent or ongoing star formation in these regions, although the rate appears to be relatively low. There is no obvious evidence of a major ongoing merger.
