This galaxy presents as an object with a generally smooth morphology. The light distribution suggests it is a roughly elliptical galaxy, as its profile appears relatively rounded with a smooth falloff. There are indications of a possible minor disturbance, such as a subtle asymmetrical tail that seems to extend slightly to the lower left. Overall, the galaxy shows a relatively centralized brightness, giving it a compact appearance. There is no clearly discernable disk structure. The color profile is trending towards bluer wavelengths, particularly concentrated in the core, indicating an increased presence of hotter, younger stars.
