The galaxy presents a morphology that is largely smooth in appearance, with a slight elongation suggestive of a weak bar or tidal distortion. The overall color profile indicates an older stellar population, though it has some presence of younger bluer stars. A brighter, more concentrated yellowish-orange central bulge dominates the galaxy's structure. A small blue disk is present on one side, with an even smaller concentration of redder stars trailing from the other side. The slight distortion is most likely due to a small gravitational interaction with another galaxy. The galaxy's half-light radius is estimated to be a few kiloparsecs. Overall, the image suggests a quiescent galaxy with a moderate stellar mass.
