The galaxy exhibits a somewhat smooth morphology, with a central bright region and a more diffuse, less luminous surrounding area. The color profile suggests a mixed stellar population, with a yellowish core potentially indicating older, more evolved stars, while bluer hues in the outer regions might signify younger stars or ongoing star formation. There appears to be some disturbance in the morphology, with possible tidal features or merging activity noticeable as deviations from a purely elliptical shape. The roundness of the galaxy suggests a more elliptical rather than disk-like structure. The galaxy's overall appearance is not perfectly symmetrical, indicating a system undergoing or having recently undergone some form of interaction or internal dynamical process.
