This galaxy presents an elliptical morphology with a smooth, centrally concentrated light distribution. There is a prominent central bulge that appears to be a yellow-orange hue, suggesting an older stellar population. The outer regions of the galaxy are less defined and display a slight elongation. There may be a faint hint of a disk structure, but it is not well-defined. Redder regions are visible within the galaxy, possibly indicative of areas of dust obscuration or pockets of more evolved stars. There is no apparent evidence of ongoing major mergers or significant tidal disturbances in this image. The galaxy appears relatively isolated and undisturbed.
