The galaxy appears to be a relatively compact system, likely a disk galaxy, exhibiting a slight elongation. The central region displays a bright, concentrated luminosity, suggesting a significant stellar population or possible AGN activity. Surrounding this core, there is a fainter, more diffuse halo, likely composed of older stars and possibly some dust. While the overall form appears relatively undisturbed, there is a hint of asymmetrical distribution of luminosity in the outer regions, potentially indicating past interactions or minor disturbances. The galaxy is blue in color, which suggests some ongoing star formation.
