The galaxy appears as a relatively smooth, elliptical-like structure with a noticeable blue hue. Its morphology suggests an early-type galaxy, possibly an elliptical or lenticular type, with a spheroidal shape that transitions into a flattened disk. There is minimal evidence of strong spiral arm structures or dust lanes typically observed in late-type galaxies.

The color gradient within the galaxy shows a more concentrated, slightly yellow-tinted core region. The surrounding galactic halo has a subtle blue tint that likely indicates the presence of younger, hotter stars. A small perturbation is visible suggesting a minor gravitational interaction or disturbance within the galaxy's structure. Overall, the galaxy seems to be at an advanced stage of evolution, and its estimated size would suggest it is a fairly large galaxy.
