The galaxy appears as a relatively smooth and rounded object with a centrally concentrated light profile. A dominant, bright, central region is visible, transitioning outward into a more diffuse, fainter halo. There is a slight elongation, but overall, the galaxy approximates a spherical shape. Based on the color indices, there may be some ongoing star formation, indicated by the bluer hues in the central region, although overall colors appear moderately red, with some yellow. There's no clear evidence of a distinct disk structure or prominent spiral arms. There are no signs of any major mergers, but there are possibly some minor disturbances. The galaxy exhibits a concentrated luminosity, with a relatively high proportion of its total light emanating from the central region. 
