The galaxy presents as an elliptical structure with a bright, concentrated central region, likely the nucleus.  Extending outward from this core is a less intensely luminous disk, oriented approximately horizontally across the field of view. The light distribution within the disk appears relatively smooth, lacking the distinct spiral arm structures seen in some galaxies.

The color distribution shows a strong central concentration of what appears to be older stars, with redder hues. Moving outwards from the center, the disk shows a ring of bluer, less red-shifted stars, likely indicative of active star formation. This hints at the potential for recent star formation. The outer regions of the galaxy fade gradually into the background. There is some slight indication of tidal disturbance along the outer edges of the disk on the top half of the image, and slightly above the bottom of the disk.
