The galaxy presents a generally smooth, elliptical morphology. It appears to have a bright, concentrated central bulge, potentially indicative of an older stellar population dominating the core. The overall colour gradient suggests a redder core gradually transitioning to slightly bluer, fainter outer regions. This could signify ongoing, albeit limited, star formation in the outskirts or possibly a more metal-poor population farther from the center. There are slight asymmetries and possibly a faint indication of a tidal feature or minor disturbance on one side. This suggests a possible past or ongoing interaction. The galaxy's elongation hints at a deviation from a perfect spherical shape. There is a clear disk visible in the galaxy which can be seen because it is being viewed at an angle.
