The galaxy presents as a fairly smooth, centrally concentrated object. There is a diffuse, extended halo surrounding a brighter core region. The overall shape is roughly elliptical, appearing relatively round. There are no obvious spiral arms or prominent dust lanes visible within the disk. There is a subtle colour gradient visible, with the core exhibiting a slightly bluer hue in comparison to the outer regions which appear more reddish. No signs of major merging events or significant tidal disturbances are evident. There are signs of some minor disturbances and the potential of tidal tails existing, but this is difficult to ascertain given the resolution of the image. The structure suggest minimal ongoing star formation.
