The galaxy appears to be a relatively smooth, elliptical-type galaxy, exhibiting a generally round morphology with a slight elongation along one axis. The light distribution suggests a concentration of older stellar populations in the core, which fades gradually towards the outer regions. The dominant color is yellowish, indicative of evolved stars and a potentially low ongoing star formation rate. There is a hint of some features, but they appear subdued and lack a structured spiral arm signature. There are no prominent tidal tails or obvious signs of a recent major merger event, although some minor disturbances in the outer structure cannot be ruled out.
