The galaxy presents a somewhat elliptical morphology, appearing largely smooth with a bright, concentrated core. The core region exhibits a bluish hue, potentially indicative of ongoing star formation or a significant population of hot, young stars. A subtle, diffuse halo surrounds the central region, fading gradually into the background. A ring-like structure may be present, indicated by a change in color surrounding the central region. There are some signs of disturbances. Overall, the galaxy appears as a moderately luminous object, with a relatively well-defined structure despite the hints of possible interaction.
