The galaxy presents as a relatively smooth, centrally concentrated object. There is a noticeable central bulge region exhibiting a bright, intense luminosity. The shape is predominantly round but not perfectly so, displaying a slight elongation. Evidence suggests a degree of disturbance in its morphology, although not a major disruptive event. The outer regions show a more diffuse nature, transitioning gradually from the bright core. The color profile exhibits a general bluer hue, suggesting a moderate level of star formation activity.
