The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. Its shape is elongated, displaying a moderate ellipticity. There is no evidence of spiral arms or a distinct disk structure, but a subtle color gradient is observed with a redder hue towards the center, possibly indicating an older stellar population concentrated at the core. Fainter, blueish light surrounds the central region, possibly pointing to a younger stellar population. No signs of ongoing major mergers or tidal disturbances are visible in the image, and the galaxy appears relatively undisturbed, without irregular features or strong asymmetries.
