The galaxy presents as a slightly elongated, disk-like structure with a bright central region. The core appears intensely luminous, exhibiting a concentrated emission profile. Surrounding the nucleus, there is evidence of a fainter, more diffuse disk component. A distinct ring-like structure is visible within the galaxy, displaying variations in color. Areas within this ring appear blue-ish, indicative of younger star formation. The outer regions of the galaxy fade into the background with hints of tidal disturbances. There appears to be a minor disturbance and possible merging event.
