The galaxy presents as a primarily smooth, elliptical structure, exhibiting a concentrated central bulge region. The overall color appears to be on the redder end of the spectrum, suggesting a relatively older stellar population. There is a subtle color gradient observable, transitioning from a slightly bluer hue in the innermost regions to a redder tint in the outer halo. No prominent spiral arms or distinct dust lanes are discernible. The overall morphology leans towards a spheroidal shape, with a high degree of roundness. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy’s form, and the image suggests there is not much current star formation.
