The galaxy presents a largely smooth morphology, appearing elliptical in shape. The light distribution is concentrated towards the center, with a bright, somewhat diffuse core. The radial light profile appears to decrease smoothly outward from the core. Faint extensions are observed, though not as concentrated towards the center. The color appears generally redder overall. Evidence of any prominent spiral structure or distinct dust lanes is absent. The morphology could suggest a relatively evolved system with a significant stellar population.
