The galaxy presents as a centrally concentrated, luminous object. It exhibits a relatively smooth morphology with a high degree of central concentration and a lack of discernable spiral arms or bar features. The color profile suggests a dominant older stellar population, indicated by the yellowish-red hue of the galaxy. There is little evidence of ongoing, intense star formation activity based on the lack of bright blue regions. The outer regions of the galaxy gradually fade into the background sky, suggesting a smooth density profile. A slight asymmetry in the outer halo might be present.
