This galaxy presents as a relatively smooth and centrally concentrated object. It appears to be elliptical in shape, exhibiting a cigar-like morphology with an aspect ratio greater than 2:1. The core region is bright and concentrated, suggesting a high density of stars. The light profile smoothly decreases from the center outwards. There's a slight blue hue to the outer edges, indicating the presence of younger, hotter stars. The redder central region possibly indicates the presence of older stellar populations. There are no signs of a strong spiral structure or tidal disturbances, but there may be a minor disturbance in the center. Overall, it looks like a large galaxy with a very slow rate of star formation.
