The galaxy presents as a centrally concentrated object, displaying a smooth, elliptical morphology. The core region exhibits a bright, relatively uniform yellow/orange hue, indicative of an older stellar population and minimal ongoing star formation. There is little evidence of spiral arm structure. The overall shape is slightly elongated, though not highly flattened. Marginal evidence suggests a possible minor disturbance, but this requires higher resolution imaging for confirmation. Based on the observed color profile, the object appears to be a massive galaxy with little on-going star formation and a significant population of older stars.
