The galaxy appears to be an elliptical galaxy, exhibiting a smooth and centrally concentrated luminosity profile. The isophotes show an intermediate ellipticity, neither perfectly round nor highly elongated. Its core region displays a yellowish hue, potentially indicating an older stellar population with lower rates of star formation and a higher abundance of evolved stars. The outer regions show a bluer color. There appears to be no evidence of significant tidal features or ongoing major mergers, although there are some hints of minor disturbances in the outskirts of the object. Overall, the galaxy is reasonably well-defined.
