The galaxy presents a largely smooth, elliptical morphology. Its core exhibits a concentrated, bright luminosity, appearing nearly spherical. The light distribution fades gradually outwards from the core, with no distinct spiral arm features apparent. A slight color gradient is observed, with the central region displaying a yellowish-white hue, suggestive of an older stellar population. The outer regions appear slightly bluer, possibly indicating the presence of younger stars, although star formation is likely occurring at a very slow rate. There is no evidence of any major ongoing merging activity or tidal disturbances that might suggest a recent interaction with another galaxy. The galaxy exhibits a generally relaxed appearance.
