The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright, yellowish-orange hue, suggesting a population of older stars and minimal ongoing star formation within the central region. The galaxy's overall shape appears moderately elliptical, with a gradual decrease in luminosity from the core outwards. There is faint blueish light in the outer regions, potentially indicative of pockets of younger stars or star formation. Overall the galaxy is a system undergoing moderate star formation. There appear to be minor disturbances in the overall structure, but it is difficult to ascertain from the imagery whether the galaxy is undergoing or has undergone a merging event.
