The galaxy presents as a relatively smooth, centrally concentrated object with a dominant bulge component. The galaxy exhibits a moderate degree of roundness, appearing more elliptical than perfectly circular. Faint, diffuse features, possibly indicative of a disk structure or tidal disturbances, are visible extending from the central region, though these are not sharply defined. Colors range from redder hues in the galaxy's core to slightly bluer tones in the outer regions. The overall morphology suggests a galaxy that has largely ceased active star formation, though low levels of star formation cannot be ruled out in the outer regions.
