The galaxy presents a morphology that suggests a transition between elliptical and spiral forms, possibly a lenticular galaxy. Its overall shape is elongated, appearing somewhat cigar-shaped, and the light distribution suggests a smooth, centrally concentrated structure with hints of a disk component. There's a notable color gradient, with a yellowish core indicating an older stellar population. The outer regions appear bluer, suggesting the presence of younger, hotter stars, potentially indicating some ongoing, albeit limited, star formation. No prominent spiral arms or other distinct features are readily apparent, supporting the classification of a galaxy with a more passive evolutionary state. There is a slight indication of minor disturbances or asymmetries within the galactic structure, but no clear signs of major mergers or interactions are seen. 
