The galaxy presents as a centrally concentrated object, appearing largely smooth with a slight elongation. The core exhibits a yellow-white hue, suggesting a population of older stars. A subtle bluish tint is visible in the outer regions, potentially indicative of younger stellar populations or ongoing star formation, albeit at a low rate. There is no visible spiral structure or prominent dust lanes. There is what appears to be another object below it in the image that is most likely an artifact, possibly a foreground star or small galaxy. This galaxy's overall morphology suggests a late-type to early-type spiral galaxy based on its light profile and features.
