The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. The core of the galaxy exhibits a bright, yellowish hue, suggesting a population of older stars. Moving outward from the core, the color shifts towards a more greenish tint, potentially indicating the presence of some younger stars or nebular emissions, though this is less pronounced. The overall structure lacks prominent spiral arms or a distinct disk. There is no sign of any major mergers or tidal disturbances and the galaxy appears to be relatively isolated. The galaxy's light is quite dim, and the red shift value indicates that it is a distant galaxy.