The galaxy presents as a centrally concentrated elliptical-like structure. It appears to be a relatively smooth object, lacking prominent spiral arms or distinct features. The color gradient suggests an older stellar population, with a yellow/orange hue dominating the central region, indicative of evolved stars. The outskirts exhibit a subtle decrease in brightness and a slight shift towards bluer tones, potentially indicating a small amount of younger star formation at the edges. The overall morphology suggests a galaxy that is in a relatively relaxed state, not showing signs of major recent mergers or significant disturbances. It exhibits intermediate roundness, not distinctly spherical, with no clear cigar shape to it.
