The galaxy presents as a roughly elliptical, moderately compact object. Its core exhibits a bright, concentrated luminosity, suggesting a significant density of stars or possible active galactic nucleus activity. The overall color appears to be biased toward the blue end of the spectrum. The light profile seems relatively smooth and featureless, lacking any prominent spiral arms or distinct morphological substructures. There is a hint of faint, extended light surrounding the central region, indicating a possible halo or outer disk component. The observed morphology is consistent with an early-type galaxy, perhaps an elliptical or lenticular type, exhibiting minimal evidence of recent or ongoing star formation.
