The galaxy presents a generally smooth and elliptical morphology. The central bulge appears prominent and exhibits a yellowish hue, suggesting an older stellar population. A faint, diffuse disk is visible, displaying a slightly bluer color indicative of more recent star formation activity, though this activity is relatively low. The galaxy is observed at an angle, appearing somewhat elongated rather than perfectly circular. There are hints of minor structural disturbances but no significant tidal features or major merger signatures are apparent.
