The galaxy presents as a relatively smooth, elliptical-like structure. Its light distribution appears concentrated toward the center, with a gradual decrease in intensity extending outwards. The galaxy exhibits a centrally dominant yellowish hue, potentially indicating an older stellar population concentrated in the core. A subtle blue tinge is visible in the outer regions, possibly indicating the presence of younger, hotter stars and ongoing star formation, though at a low rate. The overall morphology suggests a system that is neither a perfect spheroid nor a clear disk, with hints of faint, diffuse structures but no prominent spiral arms or bars are discernible. There is some indication of a minor interaction or disturbance, based on the slightly asymmetrical light distribution in the outer regions.
