The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, which appears nearly spherical. The color profile suggests a relatively uniform stellar population throughout the galaxy, with a slight bluer tinge on the outskirts that may indicate some ongoing, albeit low-level, star formation. There is no readily apparent disk structure or spiral arm features. The overall light distribution indicates that this is most likely a massive galaxy. There is no strong evidence of any major ongoing merger events or tidal disturbances. Faint traces of possible minor interaction or disturbance may be present, but require further study.
