The galaxy appears as a centrally concentrated, elliptical object with a smooth, diffuse light distribution. The core exhibits a pronounced yellowish hue, suggesting an older stellar population. The outer regions of the galaxy fade into a less defined halo with hints of reddish tones. There is no readily apparent spiral structure or significant dust lane obscuration. The general morphology suggests a relatively quiescent system with little ongoing star formation. Minor asymmetry may be present, potentially indicating a past or ongoing minor merger event, however this galaxy appears largely undisturbed.
