This galaxy presents as a relatively smooth, centrally concentrated object. The morphology appears to be largely elliptical, exhibiting a high degree of central luminosity that fades into a less concentrated halo of stars. The core displays a pronounced yellow-orange hue, indicative of an older stellar population. A subtle flattening is observed with very faint, indistinct features that do not indicate well-defined spiral arms, and a lack of any strong dust lanes. There are no obvious signs of recent major merger activity, though there appears to be some minimal asymmetric distortion and some diffuse faint blueish colors in the outer regions which may suggest minor tidal disturbances, possible satellite galaxy accretion, or regions of more recent but low star formation. The overall appearance suggests an evolved system that is largely quiescent, though with some evidence of faint recent star formation.
