The galaxy presents as a centrally concentrated object with a relatively smooth morphology. It appears nearly circular, exhibiting minimal elongation. There are no obvious signs of spiral arm structures or a prominent disk. The galaxy's color profile suggests a lack of significant ongoing star formation, leaning toward a redder hue. No major disturbances from tidal interactions or ongoing mergers are apparent; the galaxy seems isolated and settled. There is no clear presence of a galactic nucleus.
