The galaxy presents as a relatively smooth, centrally concentrated object, elongated in shape. The central region exhibits a bright, yellowish hue suggesting an older stellar population. Moving outwards from the core, the color transitions to a more diffuse bluish-white, indicating the presence of some younger stars or ongoing star formation, albeit at a low level. No distinct spiral arms or bar structures are apparent. There is no significant evidence of tidal features or major disturbances indicative of an ongoing or recent major merger. The overall morphology suggests a galaxy that is somewhere between a disk and an elliptical galaxy, possibly a lenticular galaxy, with little dust present.
