The galaxy appears as a single, relatively smooth object with a concentrated central region. The light distribution suggests an elliptical morphology, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a color gradient, appearing more yellow/red in the core, which could indicate an older stellar population. Fainter, more diffuse light extends outwards from the core, suggesting a gradual decline in stellar density. There is a slight elongation in the galaxy's shape, deviating marginally from a perfectly circular appearance. No obvious signs of recent major merger activity are apparent, and the galaxy seems largely undisturbed. Overall, the galaxy presents as a quiescent, evolved system with a high degree of central concentration.
