The galaxy appears as a generally smooth, centrally concentrated object. There is a prominent, bright core, suggesting a significant concentration of stars or potentially an active galactic nucleus.

The galaxy exhibits a flattened, disk-like morphology. Hints of disturbances are visible in the outer regions, with asymmetries in the distribution of light. These disturbances may be evidence of gravitational interactions or a minor merger.

The color profile suggests varying stellar populations. The core appears to be dominated by younger, bluer stars, while the outer regions are populated by older, redder stars. A small region of yellow emission could be due to a region of dust obscuring the stars.
