The galaxy presents as a centrally concentrated system with a generally smooth morphology. The core exhibits a high degree of luminosity, fading into a more diffuse halo. The overall shape appears to be relatively round, though there may be a slight elongation along one axis. There is little evidence of prominent spiral arms or a well-defined disk structure, however, there may be slight disturbance in the halo on the right side of the galaxy. The color profile suggests a population of older stars, potentially indicating a low rate of current star formation. No signs of major mergers are readily apparent, but the slight halo disturbance could be signs of a minor merger.
