The galaxy presents as a luminous central bulge exhibiting a golden hue, possibly indicative of an older stellar population. A slightly less luminous and more diffuse region surrounds the bulge. Faint blue tinges suggest ongoing or recent star formation within this extended region. While the galaxy appears largely smooth in overall morphology, there is subtle evidence of disturbances in the outer regions, possibly suggestive of minor tidal interactions or recent accretion events. The general shape tends toward being round, but with slight ellipticity. The redshift of the object indicates a significant distance, corresponding to a considerable size for the galaxy.
