The galaxy presents a somewhat elongated, spindle-like morphology. It appears relatively smooth, with a concentrated central bulge that graduates into a fainter, more diffuse halo. The galaxy displays a blue hue, particularly concentrated toward the center, which could indicate the presence of a younger stellar population and ongoing star formation. The outer regions are somewhat redder, suggesting an older stellar population. There is a hint of minor disturbances in the galaxy’s structure, but it is mostly a single, cohesive unit, not a major merging event. The galaxy's overall appearance suggests that it is an intermediate system, neither a pure elliptical nor a well-defined spiral, but exhibits features of both.
