The galaxy presents as a largely smooth, centrally concentrated system. The dominant feature is a bright, yellowish core that gradually fades into a less luminous halo. There's a slight elongation, but generally it appears somewhere between round and elliptical in shape. No distinct spiral arms or bar structures are visible in this image. There may be a hint of a very faint disk but it is very faint.

The color profile suggests a relatively older stellar population with a low star formation rate overall. The lack of significant blue light indicates that the presence of young, massive stars is minimal. It does not appear to be undergoing any major merging events or significant disturbances. The color varies from yellow in the center to redder hues at its furthest points, which implies a more complex stellar population as you travel outward.
