The galaxy presents a predominantly smooth morphology. A concentrated central bulge is observed, exhibiting a bright, yellowish hue. Moving outward from the core, the light gradually fades, becoming more diffuse. A faint, somewhat elongated halo surrounds the central region. There are hints of asymmetry within the outer structure, possibly indicating a minor gravitational interaction. The overall form suggests a galaxy transitioning between elliptical and lenticular classifications. Limited structural details are discernible, hinting at a relatively evolved stellar population with minimal ongoing star formation.
