The galaxy presents an elliptical morphology, appearing largely smooth in texture with a subtle elongation. The central region exhibits a pronounced concentration of light, suggesting a prominent galactic nucleus. The color distribution is not uniform; the core appears more yellow, possibly indicating an older stellar population. Proceeding outward from the center, the color shifts subtly toward redder hues. This could be indicative of ongoing, but relatively low, star formation. There is no prominent spiral structure or obvious dust lane visible, suggesting the galaxy is dominated by older stars. The galaxy appears largely undisturbed, with no obvious signs of a recent merger or tidal interactions. The overall structure indicates that the galaxy is likely an elliptical galaxy.
