The galaxy presents as an elliptical shape with a noticeable central bulge. The bulge appears to be predominantly yellow, suggesting an older stellar population. The surrounding disc exhibits a bluer hue, indicative of ongoing star formation, although not very vigorous. Overall, the galaxy appears to be relatively smooth. There are no obvious signs of major mergers or significant tidal disturbances. Faint wisps extending from the central region suggest a spiral structure, although its prominence is weak. The color gradient shows a transition from younger, bluer stars in the outer regions to older, redder stars in the core.
