The galaxy presents as a luminous, slightly elliptical, and relatively compact object. The central region displays a bright, concentrated luminosity suggesting a substantial galactic nucleus. Extending outwards from the core, a fainter, more diffuse halo is visible, with a somewhat uneven distribution of light. There appears to be some asymmetry in the shape of the galaxy, possibly indicating tidal interactions. Patches of less prominent light are visible within the disk, potentially representing areas of star formation. The overall color profile seems to be skewed towards the red end of the spectrum.
