The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, centrally bright core that fades gradually outward. There's no apparent disk structure or spiral arms. The overall color is yellowish-orange, suggesting a population of older stars and relatively little ongoing star formation. No significant dust lanes or other prominent features are visible. There is a small chance that there is a merger occurring, but it is unlikely. The galaxy appears to be well-isolated and undisturbed.
