The galaxy appears as a single, concentrated body of light with a nearly circular morphology. The overall color suggests a population of older stars, with a central concentration indicating a possible bulge. There appears to be a smooth falloff in surface brightness from the center to the outer regions, with no apparent spiral arms or other distinct features. There's no evidence of dust lanes or tidal disturbances to suggest recent interactions. The light appears to be consistent in color throughout the galaxy's structure.