The galaxy presents as a lenticular or possibly an elliptical galaxy, given its smooth, featureless appearance. It exhibits a pronounced elongated shape, suggesting a significant degree of flattening. The central region shows a concentration of light, indicating a bulge component. The color profile transitions from a relatively bluer hue at the outer edges to a yellower and redder core, potentially indicating a radial gradient in stellar populations and dust content. The blue outskirts hint at the presence of younger stars or ongoing star formation, while the redder core suggests an older stellar population. No distinct spiral arms or bar features are discernible in the image, consistent with a lack of significant recent star formation. There appears to be no major ongoing merger activity or significant tidal disturbances. The overall structure points to a galaxy that has largely completed its disk formation and is in a more quiescent evolutionary state.
