This galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears largely uniform without prominent spiral arms or a distinct bar structure. There is a slight elongation visible, suggesting a deviation from perfect sphericity. The central region appears to be brighter and exhibits a yellowish hue, potentially indicating an older stellar population. Fainter bluish tints are present in the outer regions, suggesting some ongoing star formation, albeit at a modest level. There is no clear evidence of any major mergers or tidal disturbances in the immediate vicinity. Overall, the morphology points towards a galaxy that is well evolved and relatively quiescent.
