The galaxy exhibits a morphology that appears largely smooth and centrally concentrated. There is a slight elongation. The object exhibits an overall yellowish-white hue. Subtle, low-level features suggest potential disturbances or faint spiral structures, but these are not well-defined. The color suggests a population of older stars. No strong dust lanes or prominent star-forming regions are readily apparent. The relative lack of blue light indicates suppressed recent star formation activity. Overall the galaxy is relatively undisturbed.
