The galaxy appears as a single, somewhat irregular object with a smooth overall light distribution. It exhibits a slightly elongated morphology, appearing as a flattened spheroid rather than a perfect circle. There is a subtle color gradient visible within the galaxy; the central region appears more yellow, suggesting an older stellar population, while the outer regions have hints of bluer light, possibly indicating more recent star formation. The galaxy does not show any prominent spiral arm structures, and the light is mostly centrally concentrated. However, there is an indication of a small, secondary component or merging object to one side of the main galaxy body. This may suggest a recent or ongoing minor merger event, or at least some gravitational disturbance. The galaxy appears to have a relatively quiescent star formation rate, based on the overall color and morphology.
