The galaxy presents as a generally smooth and rounded structure, consistent with an elliptical morphology. The central region exhibits a strong concentration of light, appearing nearly spherical with a yellowish hue, likely indicating an older stellar population. Moving outward from the core, the light intensity decreases gradually, and the color becomes slightly redder. There are no visible spiral arms or prominent dust lanes discernible in the image. The galaxy appears relatively undisturbed, lacking any obvious signs of tidal interactions or major mergers. A very slight asymmetry is present, possibly a faint, unresolved feature. Overall, the appearance suggests a relatively evolved galaxy with a dominant spheroidal component.
