The galaxy presents as a multi-component system. A dominant, luminous, spheroid component is observed, exhibiting a smooth, rounded morphology. The core of this spheroid is a slightly more intense orange hue, gradually fading to a yellowish halo surrounding it.

Below the spheroid, a secondary, elongated structure is visible. This component is less luminous and displays a flattened, disk-like morphology. The color gradient within this disk ranges from redder regions to a more diffuse bluish tint on its outer edges. It is oriented at an angle relative to our line of sight. 

There appears to be some level of gravitational interaction between the spheroid and the disk component. While the spheroid appears relatively undisturbed, the disk exhibits some irregularities in its structure, possibly indicating minor tidal distortions.

Overall, the galaxy appears to be a mid-sized system with a mixture of evolved stellar populations in the spheroid and some evidence of ongoing star formation in the disk. The system exhibits a complex morphology, potentially indicative of an ongoing or past minor merger event.
