The galaxy presents as a somewhat elliptical object, exhibiting a smooth morphology. The color profile suggests a centrally concentrated yellowish hue, potentially indicative of an older stellar population dominating the core. The outer regions display a bluer tint, hinting at the presence of younger stars, although the smooth texture does not lend itself to the easy visibility of defined spiral arms or star-forming regions. The galaxy's light appears relatively undisturbed, with no obvious signs of major ongoing mergers or tidal interactions. There may be minor asymmetry in the overall shape, suggesting the possibility of minor disturbances, but it does not appear to be a major merger event. Overall, the morphology points to a galaxy with a significant spheroidal component.
