The galaxy appears as a relatively smooth, centrally concentrated object with a dominant yellowish hue. It exhibits a slight elongation, deviating marginally from a perfectly circular morphology. There are no discernible spiral arm structures or prominent dust lanes visible at this resolution. The light distribution suggests a bulge-dominated system, potentially an elliptical galaxy or a lenticular galaxy seen at a considerable distance. There is a slight hint of a disturbed structure or a possible minor interaction with a faint object, indicating a possible merger event. Given its color, the galaxy likely contains a population of older stars with low ongoing star formation. The overall form suggests a galaxy of significant mass.
