The galaxy exhibits a generally smooth morphology, with a bright, centrally concentrated core region. This core displays a near-spherical shape, indicating a possible spheroidal component such as a bulge. 

The galaxy's overall color profile suggests a mixture of stellar populations. It shows a slightly bluer hue towards the center.

There is a hint of possible minor disturbance in the overall symmetry of the galaxy, but no major disruptions or signs of ongoing merger activity are immediately apparent. Based on this assessment, it is likely this is not a strong interaction.
