The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round in shape with a slight elongation. There's no clear evidence of spiral arms or a distinct disk structure. A prominent, bright central bulge is visible, suggesting a higher concentration of older stars and potentially a supermassive black hole. The color gradient indicates a mixture of stellar populations, with the central bulge exhibiting a redder hue, likely indicative of older, cooler stars, while the outer regions show a slightly bluer tint. The light distribution appears smooth, with a gradual decrease in brightness from the center outwards, showing no significant signs of major disturbances or ongoing merger activity. There's no significant dust lane apparent, suggesting that the galaxy is relatively dust-poor.
